Weekly Space Hangout – Mar 31, 2017: The IDATA Project and Afterglow Access

Host: Fraser Cain (@fcain)

Special Guest:
This week’s special guests are Timothy Spuck, Kathryn Meredith, Dr. James Hammerman and Andreas Stefik of the Innovators Developing Accessible Tools for Astronomy (IDATA) Project Team. The IDATA project aims to design and develop Afterglow Access, a new software tool that will expand accessibility beyond touch, making the universe more accessible to those with visual impairments.

Yerkes Outreach website
Tim Spuck (email: [email protected]) (Associated Universities Inc. STEM Education Development Officer and IDATA PI) currently serves as PI on three NSF supported programs including, Innovators Developing Accessible Tools for Astronomy, the Chile-US Astronomy Education Outreach Summit, and the Astronomy in Chile Educator Ambassadors Program. Tim also remains active within the amateur astronomy community, has directed numerous outreach efforts, and led several small-scale observatory design and construction projects. He earned his Masters degree in Science Education from Clarion University or PA, and is completing his Ed.D. in Curriculum & Instruction at West Virginia University.

Kate Meredith (Yerkes Observatory – University of Chicago, Director of Education Outreach, and IDATA Project Educator) has engaged in curriculum development and project management for the Zooniverse, the Sloan Digital Sky Survey, the Lawrence Hall of Science, the Adler Planetarium Space and Science Museum, and Skynet Junior Scholars (University of Chicago Yerkes Observatory). Kate is passionate about programs that bring authentic research science to learners of all ages, languages, and abilities. As Education Lead on the IDATA project, Kate looks forward to being part of the team that takes accessibility to the next level by creating vision-neutral data acquisition and analysis tools as well as the instructional materials needed to teach new users how to use and apply those tools.

Dr. James K. L. Hammerman (TERC, Co-Director of SEEC and Senior Researcher and Evaluator, IDATA Co-PI) currently leads external evaluations for several projects, including an immersive computer environment for conducting experiments to explore causality and ecology, a state-wide initiative to engage rural youth in computing through programming an online game, and an effort to improve pedagogy among university STEM faculty. Jim has designed, implemented, and researched mathematics and science education curricula and professional development programs, as well as technology tools that support inquiry-oriented learning. Jim is especially interested in adult developmental differences in professional development, data and statistics learning, online and software tools that support exploration, and supporting deeper learning and more reflective practice in professional communities.

Andreas Stefik (University of Nevada – Las Vegas, Assistant Professor of Computer Science and IDATA Co-PI) – For the last decade, Dr. Stefik has been creating technologies that make it easier for people, including those with disabilities, to write computer software. With grants from the National Science Foundation, he helped establish the first national educational infrastructure for blind or visually impaired students to learn computer science. He is the inventor of Quorum, the first evidence-oriented programming language. As part of his work, he is a PI on the NSF-funded AccessCS10K grant that is helping CS 10K projects prepare K-12 teachers to be more inclusive in their computing courses with students with disabilities. Most recently, Dr. Stefik was honored with the 2016 White House Champions of Change award in computer science education.

Accessibility links mentioned in the show:
Quorum Language
CS for All
CS for All links

Guests:
Morgan Rehnberg (MorganRehnberg.com / @MorganRehnberg)

Their stories this week:

SpaceX relaunches a rocket for the first time

NASA fleshed out its human Mars program

We use a tool called Trello to submit and vote on stories we would like to see covered each week, and then Fraser will be selecting the stories from there. Here is the link to the Trello WSH page (http://bit.ly/WSHVote), which you can see without logging in. If you’d like to vote, just create a login and help us decide what to cover!

If you would like to join the Weekly Space Hangout Crew, visit their site here and sign up. They’re a great team who can help you join our online discussions!

If you’d like to join Fraser and Paul Matt Sutter on their tour to Iceland in February 2018, you can find the information at astrotouring.com.

We record the Weekly Space Hangout every Friday at 12:00 pm Pacific / 3:00 pm Eastern. You can watch us live on Universe Today, or the Universe Today YouTube page

ARCA Unveils the World’s first Single-Stage-to-Orbit Rocket

Artist's impression of the Haas 2CA deployed to orbit. Credit: ARCA

Since the beginning of the Space Age, scientists have relied on multi-stage rockets in order to put spacecraft and payloads into orbit. The same technology has allowed for missions farther into space, sending robotic spacecraft to every planet in the Solar System, and astronauts to the Moon. But looking to the future, it is clear that new ideas will be needed in order to cut costs and expand launch services.

Hence why the ARCA Space Corporation has developed a concept for a single-stage-to-orbit (SSTO) rocket. It’s known as the Haas 2CA, the latest in  a series of rockets being developed by the New Mexico-based aerospace company. If all goes as planned, this rocket will be the first SSTO rocket in history, meaning it will be able to place payloads and crew into Earth’s orbit relying on only one stage with one engine.

The rocket was unveiled on Tuesday, March 28th, at their company headquarters in Las Cruces. The rocket is currently seeking FAA approval, and ARCA is working diligently to get it ready for its test launch in 2018 – which will take place at NASA’s Wallops Flight Facility located on Virginia’s eastern shore. If successful, the company hopes to use this rocket to deploy small satellites to orbit in the coming decade.

Artist’s impression of the Haas 2C rocket ascending into orbit. Credit: ARCA

Established in 1999 by a group of Romanian rocket enthusiasts (led by company CEO Dumitru Popescu), ARCA’s original focus was on balloon-launched rockets. In the course of the company’s history, ARCA has launched two stratospheric rockets, four large scale stratospheric balloons, and has been awarded some lucrative governmental contracts to test aerospace and space exploration technologies.

In 2003, the company joined the $10 million Ansari X Prize Competition and began work on their first demonstrator rocket. Known as the Demonstrator 2B – a single stage suborbital rocket – the rocket was successfully launched on September 9th, 2004, from Cape Midia Air Force Base. In the years that followed, they expanded their repertoire to include other concepts – like the Helen rocket, the Stabilo crewed vehicle, and the Excelsior Aerospike.

In 2013, ARCA was contracted by the European Space Agency (ESA) to create a Drop Test Vehicle (DTV) that would test the atmospheric deceleration parachutes being used by the Schiaperelli lander (as part of the ExoMars mission). Being the same weight and using the same parachute deployment systems as Schiaperelli, the DTV conducted a freefall exercise which simulated the dynamic pressure conditions of entering the Martian atmosphere

In that same year, ARCA relocated to New Mexico, where they have continued working on their rocket series and other aerospace ventures from their headquarters at the Las Cruces Airport. It was here that they introduced the Haas rocket series – named in honor of Austrian-Romanian rocketry pioneer Conrad Haas – which now consists of the Haas 2B and 2C rockets.

The Haas 2CA rocket berthed at ARCA’s headqaurters at Las Cruces Air Port in Las Cruces, New Mexico. Credit: ARCA

The 2B is a proven concept, designed for suborbital flight for the sake of space tourism. But as of this week, the 2C is now part of ARCA’s rocket family. Relying on single stage and single Executor engine, this rocket will small satellites into orbit. The rocket is fueled by hydrogen peroxide and kerosene (which combines to create a nontoxic fuel), and measures (53 feet) long and (5 feet) in diameter.

The 2C weights about 550 kg (1210 pounds) empty, and 16280 kg (35,887 pounds) when fully fueled. It will also be able to provide 22900 kg (50,500 lbs) of thrust at sea level, and about 33,565 kg (74,000 lbs) in a vacuum. In this configuration, the rocket is capable of delivering 100kg (220lbs) to Low Earth Orbit (LEO), at a cost of $1 million per launch (or $10,000/kg; $4,545/lb).

This several times less what SpaceX can do with its Falcon 9 rocket, which can deliver 22,800 km payloads to orbit for $62 million a launch – which works out to about $2719/kg or $1233/lb. However, one must take into account that the Falcon 9 is a heavier launch vehicle, and that there are additional issues that come into play where larger launch vehicles are concerned. As Dumitru Popescu told Universe Today via email:

“With the Haas 2C, the customer can launch on the desired orbit parameter, when he/she wants. Basically, the launch will be tailored on the customer needs. A more fair comparison will be between the Haas 2CA and Falcon 1 and Electron. Falcon 1 had a launch cost of $6.7 millions for a proposed payload of 670kg, or a demonstrated one of 180kg. In the best case scenario, this leads us to the same price of $10,000/kg. In the case of the Electron rocket, the cost per launch is $4.9 million for a 150kg payload. This leads us to a price of a $32.600/kg. Falcon 1, Electron, Haas 2CA have their market and a comparison with a big launcher isn’t fair in my opinion. Overall, if we will be able to keep this price, the Haas 2CA, at $1 million/launch will become the cheapest launcher in history.”

Artist’s impression of the Haas 2C rocket, shown in its launch (top) and deployment configurations (bottom). Credit: ARCA

In addition, the Haas 2C rocket benefits from the fact that it is cheaper and easier to manufacture, and that it’s SSTO configuration offers greater flexibility and reliability. 

“In the case of staged rockets, we are literally talking about more rockets combined in one vehicle to achieve orbit,” said Popsecu. “It is definitely more cost effective to operate one rocket than a vehicle made of multiple rockets, as it requires less time, less qualified manpower and less demanding transport and launch operations. The SSTO may also offer the possibility to launch from an inland spaceport, as there are no first stages that will fall on the ground after burnout.”

To prepare the rocket for its 2018 launch, ARCA is currently collaborating with NASA through its Cooperative Opportunity Program and with the help of the Ames, Kennedy, Marshall,  Stennis, and Johnson Space Centers. Popescu is also entering into discussions with the New Mexico Spaceport Authority to conduct launches from Spaceport America, and is looking to secure a partnership with a US defense agency.

If all goes well, this little aerospace company will be making spaceflight history. As Popescu said in a company press release:

“When the Haas 2CA rocket launches, it will be the first rocket in history to place itself entirely into orbit. This opens new frontiers for exploration of the Solar System as the rocket can be refueled in-orbit and re-utilize its aerospike engine thus eliminating the need for additional upper stages. After the full qualification, the vehicle could be operated from inland spaceports as there are no stages that fall on the ground at burnout. Staged rockets, even though they provide more payload performance for the same takeoff mass, are less reliable because of an increased number of parts due to flight events requested by staging and ignition of the upper stage engine. Also, staged rockets are deemed to be more expensive because they are literally made up of more than one rocket. Manufacturing and assembling more rockets in one launcher requires more, time, money, and personnel. The SSTO technology, once implemented, will increase the space flight responsiveness and lower the cost to values expected by the industry for decades. This rocket will also be the fastest vehicle to reach orbit, taking less than 5 minutes.”

In addition, the aerospace industry will have another company looking to lower the costs of launches and expanding domestic launch capability. Be sure to check out the company’s video detailing the Haas 2C and its unique characteristics:

Further Reading: ARCA

SpaceX Accomplishes American ‘Science Triumph’ with ‘Mind Blowing’ Historic 2nd Launch and Landing of Used Rocket

The ‘used’ SpaceX Falcon 9 launches the SES-10 telecomsat to orbit from historic Launch Complex 39A as it zooms past US Flag by the countdown clock at NASA’s Kennedy Space Center in Florida at 6:27 p.m. EDT on March 30, 2017. Credit: Ken Kremer/Kenkremer.com
The ‘used’ SpaceX Falcon 9 launches the SES-10 telecomsat to orbit from historic Launch Complex 39A as it zooms past US Flag by the countdown clock at NASA’s Kennedy Space Center in Florida at 6:27 p.m. EDT on March 30, 2017. Credit: Ken Kremer/Kenkremer.com

KENNEDY SPACE CENTER, FL – SpaceX accomplished an American ‘Science Triumph’ with today’s “Mind Blowing” and history making second launch and landing of a previously flown Falcon 9 booster that successfully delivered a massive and powerful Hi Def TV satellite to orbit for telecom giant SES from the Kennedy Space Center. Note: Breaking News story being updated.

The milestone SpaceX mission to refly the first ever ‘used rocket’ blasted off right on time at dinnertime today, Thursday, March 30, at 6:27 p.m. EDT. It carried the SES-10 telecommunications payload to orbit atop a ‘Flight-Proven’ Falcon 9 rocket from seaside Launch Complex 39A at NASA’s Kennedy Space Center in Florida.

The recycled Falcon delivered the nearly six ton SES-10 satellite to geostationary transfer orbit where it will provide significantly improved TV, voice, data and maratime service to over 37 million customers across Central and South America.

The daring mission to relaunch a used booster dubbed ‘Flight-Proven’ seems like its straight out of a science fiction thriller.

Yet today’s stellar results fully vindicates billionaire SpaceX CEO and Chief Designer Elon Musk’s bold vision to slash launch costs by recovering and reusing spent first stage rockets from his firms Falcon 9 launch vehicle.

“My mind is blown,” Musk said in post launch remarks at the KSC press site. “This is one of the coolest things ever.”

“We just had an incredible day today – the first re-flight of an orbital-class booster.”

“It did its mission perfectly, dropped off the second stage, came back and landed on the drone ship, right on the bullseye. It’s an amazing day, I think, for space as a whole, for the space industry.”

Recycled SpaceX Falcon 9 skyrockets to orbit with SES-10 telecomsat from historic Launch Complex 39A as it zooms past US Flag by the countdown clock at NASA’s Kennedy Space Center in Florida at 6:27 p.m. EDT on March 30, 2017. Credit: Ken Kremer/Kenkremer.com

For the first time in world history a recovered and ‘Flight-Proven’ rocket has actually launched on a second mission and not only roared aloft but survived intact all the way to its intended orbit and delivered a second satellite to orbit for a paying customer- in this case the commercial TV broadcast satellite provider SES- one of the world’s largest.

“This will rock the space industry,” said SES CTO Martin Halliwell at the post launch media briefing. “And SpaceX already has!”

“We are confident in this booster,” Halliwell told me at a prelaunch press briefing on March 28.

“There is not a huge risk,” Halliwell stated emphatically. “In this particular case we know that the reusability capability is built into the design of the Falcon 9 vehicle.”

Reflown SpaceX Falcon 9 soars to orbit with SES-10 telecomsat from historic Launch Complex 39A at NASA’s Kennedy Space Center in Florida at 6:27 p.m. EDT on March 30, 2017. Credit: Ken Kremer/Kenkremer.com

This recycled Falcon 9 first stage booster had initially launched in April 2016 for NASA on the SpaceX Dragon CRS-8 resupply mission to the International Space Station (ISS) under contract for the space agency.

Furthermore, after the 156 foot tall first stage booster completed its primary mission task, SpaceX engineers successfully guided it to a second landing on the tiny OCISLY drone ship for a soft touchdown some eight and a half minutes after liftoff.

OCISLY had left Port Canaveral several days ahead of the March 30 launch and was prepositioned in the Atlantic Ocean some 400 miles (600 km) off the US East coast, just waiting for the boosters 2nd history making approach and pinpoint propulsive soft landing.

It thus became the first booster in history to launch twice and land twice.

SpaceX CEO and Chief Designer Elon Musk and SES CTO Martin Halliwell exuberantly shake hands of congratulation following the successful delivery of SES-10 TV comsat to orbit using the first reflown and flight proven booster in world history at the March 30, 2017 post launch media briefing at NASA’s Kennedy Space Center in Florida. Credit: Ken Kremer/Kenkremer.com

And this magnificent achievement was accomplished through the dedication and hard work of engineers and scientists who benefited from the American education system that cultivated and nurtured their talents – like generations before them – and that we as a country must continue to support and fortify with reliable and ample research and development (R&D) and educational funding – now and in the future – if we wish to remain leaders in science and space.

The entire Falcon 9/SES-10 launch and landing was broadcast live on the SpaceX hosted webcast.

SpaceX Falcon 9 recycled rocket carrying SES-10 telecomsat raised erect atop Launch Complex 39A at the Kennedy Space Center as seen from inside the pad ahead of liftoff slated for 6:27 p.m on 30 Mar 2017 on world’s first reflight of an orbit class rocket. Credit: Ken Kremer/Kenkremer.com

Watch for Ken’s continuing coverage direct from onsite at the Kennedy Space Center press site and Cape Canaveral Air Force Station.

Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.

Ken Kremer

………….

Learn more about SpaceX SES-10, EchoStar 23 and CRS-10 launches to ISS, ULA SBIRS GEO 3 launch, GOES-R launch, Heroes and Legends at KSCVC, OSIRIS-REx, InSight Mars lander, Juno at Jupiter, SpaceX AMOS-6, ISS, ULA Atlas and Delta rockets, Orbital ATK Cygnus, Boeing, Space Taxis, Mars rovers, Orion, SLS, Antares, NASA missions and more at Ken’s upcoming outreach events at Kennedy Space Center Quality Inn, Titusville, FL:

Mar 31, Apr 1: “SpaceX SES-10, EchoStar 23, CRS-10 launch to ISS, ULA Atlas SBIRS GEO 3 launch, GOES-R weather satellite launch, OSIRIS-Rex, SpaceX and Orbital ATK missions to the ISS, Juno at Jupiter, ULA Delta 4 Heavy spy satellite, SLS, Orion, Commercial crew, Curiosity explores Mars, Pluto and more,” Kennedy Space Center Quality Inn, Titusville, FL, evenings

SpaceX Falcon 9 recycled rocket carrying SES-10 telecomsat poised atop Launch Complex 39A at the Kennedy Space Center ahead of liftoff slated for 6:27 p.m. on 30 Mar 2017 on world’s first reflight of an orbit class rocket. Credit: Ken Kremer/Kenkremer.com

The SES-10 satellite was manufactured by Airbus Defence & Space and is based on the Eurostar E3000 platform. It will operate in geostationary orbit.Credit: SES/Airbus
SpaceX Falcon 9 booster from Thaicom-8 launch on May 27, 2016 arrives at mouth of Port Canaveral, FL on June 2, 2016. Credit: Ken Kremer/kenkremer.com

Solar Probe Plus Will ‘Touch’ The Sun

NASA's Solar Probe Plus will enter the sun's corona to understand space weather using a Faraday cup developed by the Smithsonian Astrophysical Observatory and Draper. Credit: NASA/Johns Hopkins University Applied Physics Laboratory

Coronal Mass Ejections (aka. solar flares) are a seriously hazardous thing. Whenever the Sun emits a burst of these charged particles, it can play havoc with electrical systems, aircraft and satellites here on Earth. Worse yet is the harm it can inflict on astronauts stationed aboard the ISS, who do not have the protection of Earth’s atmosphere. As such, it is obvious why scientists want to be able to predict these events better.

For this reason, the Smithsonian Astrophysical Observatory and the Charles Stark Draper Laboratory – a Cambridge, Massachusetts-based non-profit engineering organization – are working to develop specialized sensors for NASA’s proposed solar spacecraft. Launching in 2018, this spacecraft will fly into the Sun atmosphere and “touch” the face of the Sun to learn more about its behavior.

This spacecraft – known as the Solar Probe Plus (SPP) – is currently being designed and built by the Johns Hopkins University Applied Physics Laboratory. Once it is launched, the SPP will use seven Venus flybys over nearly seven years to gradually shrink its orbit around the Sun. During this time, it will conduct 24 flybys of the Sun and pass into the Sun’s upper atmosphere (corona), passing within 6.4 million km (4 million mi) of its surface.

At this distance, it will have traveled 37.6 million km (23.36 million mi) closer to the Sun than any spacecraft in history. At the same time, it will set a new record for the fastest moving object ever built by human beings – traveling at speeds of up to 200 km/sec (124.27 mi/s). And last but not least, it will be exposed to heat and radiation that no spacecraft has ever faced, which will include temperatures in excess of 1371 °C (2500 °F).

As Seamus Tuohy, the Director of the Space Systems Program Office at Draper, said in a CfA press release:

“Such a mission would require a spacecraft and instrumentation capable of withstanding extremes of radiation, high velocity travel and the harsh solar condition—and that is the kind of program deeply familiar to Draper and the Smithsonian Astrophysical Observatory.”

In addition to being an historic first, this probe will provide new data on solar activity and help scientists develop ways of forecasting major space-weather events – which impact life on Earth. This is especially important in an age when people are increasingly reliant on technology that can be negatively impacted by solar flares – ranging from aircraft and satellites to appliances and electrical devices.

According to a recent study by the National Academy of Sciences, it is estimated that a huge solar event today could cause two trillion dollars in damage in the US alone – and places like the eastern seaboard would be without power for up to a year. Without electricity to provide heating, utilities, light, and air-conditioning, the death toll from such an event would be significant.

As such, developing advanced warning systems that could reliably predict when a coronal mass ejection is coming is not just a matter of preventing damage, but saving lives. As Justin C. Kasper, the principal investigator at the Smithsonian Astrophysical Observatory and a professor in space science at the University of Michigan, said:

“[I]n addition to answering fundamental science questions, the intent is to better understand the risks space weather poses to the modern communication, aviation and energy systems we all rely on. Many of the systems we in the modern world rely on—our telecommunications, GPS, satellites and power grids—could be disrupted for an extended period of time if a large solar storm were to happen today. Solar Probe Plus will help us predict and manage the impact of space weather on society.”

To this end, the SPP has three major scientific objectives. First, it will seek to trace the flow of energy that heats and accelerates the solar corona and solar wind. Second, its investigators will attempt to determine the structure and dynamics of plasma and magnetic fields as the source of solar wind. And last, it will explore the mechanisms that accelerate and transport energetic particles – specifically electrons, protons, and helium ions.

To do this, the SPP will be equipped with an advanced suite of instruments. One of the most important of these is the one built by the Smithsonian Astrophysical Observatory with technical support from Draper. Known as the Faraday Cup – and named after famous electromagnetic scientists Michael Faraday – this device will be operated by SAO and the University of Michigan in Ann Arbor.

Designed to withstand interference from electromagnetic radiation, the Farady Cup will measure the velocity and direction of the Sun’s charged particles, and will be only two positioned outside of the SPP’s protective sun shield – another crucial component. Measuring 11.43 cm (4.5 inches) thick, this carbon composition shield will ensure that the probe can withstand the extreme conditions as it conducts its many flybys through the Sun’s corona.

Naturally, the mission presents several challenges, not the least of which will be capturing data while operating within an extreme environment, and while traveling at extreme speeds. But the payoff is sure to be worth it. For years, astronomers have studied the Sun, but never from inside the Sun’s atmosphere.

By flying through the birthplace of the highest-energy solar particles, the SPP is set to advance our understanding of the Sun and the origin and evolution of the solar wind. This knowledge could not only help us avoid a natural catastrophe here on Earth, but help advance our long-term goal of exploring (and even colonizing) the Solar System.

Further Reading: CfA

The Ever-Working Mars Orbiter Passes 50,000 Orbits

This image is a mosaic of all the images captured by the Context Camera (CTX) on NASA's Mars Reconnaissance Orbiter. The CTX has imaged over 99% of the Martian surface. Image: NASA/JPL-Caltech/MSSS

Most of us never do one thing 50,000 times in our life. So for NASA’s Mars Reconnaissance Orbiter (MRO), completing 50,000 orbits around the red planet is a big deal. And, it only took 10 years to do so.

The MRO could be called one of NASA’s flagship missions. It’s presence in orbit around Mars has helped open up our understanding of that planet immensely. And it’s done so while providing us a steady stream of eye candy.

This recent image from MRO’s HiRise camera shows dune structure inside an impact crater. Image: NASA/JPL/University of Arizona

MRO was launched in 2005 and reached Mars orbit in March, 2006. After 10 years at work, it has accomplished a lot. In a recent press release, NASA calls the MRO “the most data-productive spacecraft yet.” Though most of us might know the orbiter because of it’s camera, the High-Resolution Imaging Science Experiment (HiRise), the MRO actually has a handful of other instruments that help the orbiter achieve its objectives. In broad terms, those objectives are:

  • to study the history of water on Mars
  • to look at small scale features on the surface, and identify landing sites for future Mars missions
  • to act as a communications relay between Mars and Earth

MRO investigating Martian water cycle – This artist’s concept represents the “Follow the Water” theme of NASA’s Mars Reconnaissance Orbiter mission. The orbiter’s science instruments monitor the present water cycle in the Mars atmosphere and the associated deposition and sublimation of water ice on the surface, while probing the subsurface to see how deep the water-ice reservoir extends. Image: By NASA/JPL/Corby Waste – http://photojournal.jpl.nasa.gov/catalog/PIA07241 (image link), Public Domain, https://commons.wikimedia.org/w/index.php?curid=374810 (Larger image here.

MRO’s HiRise camera gets all the glory, but it’s another onboard camera, the Context Camera (CTX), that is the real workhorse. The CTX is a much lower resolution than the HiRise, but its file sizes are much more manageable, an important consideration when every file has to travel from Mars to Earth—an average distance of about 225 million km.

CTX has captured 90,000 images so far in MRO’s mission, and each one captures details smaller than a tennis court. In the course of the mission so far, CTX has images that cover 99.1% of the Martian surface. Over 60% of the planet has been covered twice.

“Reaching 99.1-percent coverage has been tricky…” – Context Camera Team Leader Michael Malin

“Reaching 99.1-percent coverage has been tricky because a number of factors, including weather conditions, coordination with other instruments, downlink limitations, and orbital constraints, tend to limit where we can image and when,” said Context Camera Team Leader Michael Malin of Malin Space Science Systems, San Diego.

Malin said, “Single coverage provides a baseline we can use for comparison with future observations, as we look for changes. Re-imaging areas serves two functions: looking for changes and acquiring stereoscopic views from which we can make topographic maps.”

Because the CTX captures image of the same surface areas twice, it documents changes on the surface. There have been over 200 instances of impact craters appearing in a second image of the same area. Scientists have used this to calculate the rate that meteorites impact Mars.

The instruments on board the MRO work as a team. The CTX can capture images of areas of interest, and the HiRise can be used for higher-resolution images of the same area. By locating fresh impact craters, then studying them more closely, the MRO has helped discover the presence of what looked like sub-surface ice on Mars. A third instrument, the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM), confirmed the presence of ice.

The CTX is the workhorse camera, and the HiRise is the diva, but MRO actually has a third camera: the Mars Color Imager (MARCI). MARCI is a very low resolution camera compared to the others. It’s also a wide-angle camera with really only one purpose: characterizing Martian weather. Every day, MARCI takes about 84 images which together create a daily global map of Mars. You can see a weekly Martian weather report from MARCI here.

The MRO recently manoeuvered itself into position for its next task—helping the InSight Lander. The MRO must receive critical radio transmissions from NASA’s InSight Lander as it descends to Mars. Insight will use its instruments to examine the interior of Mars for clues to how rocky planets form. Not only did MRO help find a landing spot for Insight, but it will hold the lander’s hand as it descends, and it will act as a data relay.

“After 11 and a half years in flight, the spacecraft is healthy and remains fully functional.” – MRO Project Manager Dan Johnston.

There’s no end in sight for the MRO. It just keeps going and going, and fulfilling its mission objectives on a continuing basis. “After 11 and a half years in flight, the spacecraft is healthy and remains fully functional,” said MRO Project Manager Dan Johnston at NASA’s Jet Propulsion Laboratory, Pasadena, California. “It’s a marvelous vehicle that we expect will serve the Mars Exploration Program and Mars science for many more years to come.”

SpaceX Attempting Launch of 1st Orbit Class Recycled Rocket March 30 – Watch Live

SpaceX Falcon 9 recycled rocket carrying SES-10 telecomsat raised erect atop Launch Complex 39A at the Kennedy Space Center as seen from inside the pad ahead of liftoff at 6:27 p.m on 30 Mar 2017 on world’s first reflight of an orbit class rocket. Credit: Ken Kremer/Kenkremer.com

SpaceX Falcon 9 recycled rocket carrying SES-10 telecomsat raised erect atop Launch Complex 39A at the Kennedy Space Center as seen from inside the pad ahead of liftoff slated for 6:27 p.m on 30 Mar 2017 on world’s first reflight of an orbit class rocket. Credit: Ken Kremer/Kenkremer.com

KENNEDY SPACE CENTER, FL – The moment of truth is rapidly approaching as SpaceX attempts the world’s first reflight of an orbital class rocket later today, Thursday, March 30, with the firms Falcon 9 standing proudly at historic launch complex 39A at NASA’s Kennedy Space Center in Florida – ready to deliver an advanced TV broadcast satellite to orbit for the America’s for telecom giant SES.

If successful, the launch will mightily advance billionaire SpaceX CEO Elon Musk’s bold vision to slash launch costs by recovering and reusing spent first stage rockets from his firms Falcon 9 launch vehicle.

“The SES-10 mission will mark a historic milestone on the road to full and rapid reusability,” say Space officials.

“We are confident in this booster,” SES CTO Martin Halliwell told Universe Today at a press briefing on March 28.

SpaceX Falcon 9 recycled rocket carrying SES-10 telecomsat poised atop Launch Complex 39A at the Kennedy Space Center ahead of liftoff slated for 6:27 p.m. on 30 Mar 2017 on world’s first reflight of an orbit class rocket. Credit: Ken Kremer/Kenkremer.com

The milestone SpaceX mission destined to refly the first ever ‘used rocket’ is slated for lift off on Thursday, March 30, at 6:27 p.m. EDT carrying the SES-10 telecommunications payload to orbit atop a ‘Flight-Proven’ Falcon 9 rocket from seaside Launch Complex 39A at NASA’s Kennedy Space Center in Florida.

So, if you want to witness this truly magnificent event in space history with your own eyes, there’s only a few hours left for you to ‘Get Your Ass to KSC!’ to paraphrase Apollo 11 moonwalker Buzz Aldrin.

The nearly six ton SES-10 satellite will provide significantly improved TV, voice, data and maratime service to over 37 million customers across Central and South America.

Eventually, Musk hopes to help establish a ‘City on Mars’ by building Interplanetary Colonial Transporters to transport human settlers to live on the Red Planet – the most Earth-like world in our Solar System.

You can watch the launch live on a SpaceX dedicated webcast starting about 20 minutes prior to the 6:27 pm EDT or 10:27 pm UTC liftoff time.

The two and a half hour launch window closes at 9:57 p.m. EDT.

Watch the SpaceX broadcast live at: SpaceX.com/webcast

The weather outlook is glorious along the Florida Space Coast with an 80% chance of favorable conditions at launch time in the latest AF prognosis.

However for the back-up launch date on Friday, the outlook worsens considerable to only 40% favorable.

“This thing is good to go!” Halliwell told me.

The SES-10 satellite was manufactured by Airbus Defence & Space and is based on the Eurostar E3000 platform. It will operate in geostationary orbit.Credit: SES/Airbus

The Falcon 9 booster to be recycled was initially launched in April 2016 for NASA on the SpaceX Dragon CRS-8 resupply mission to the International Space Station (ISS) under contract for the space agency.

The 156 foot tall first stage was recovered about eight and a half minutes after liftoff via a pinpoint propulsive soft landing on an tiny ocean going droneship prepositioned in the Atlantic Ocean some 400 miles (600 km) off the US East coast.

If all goes well SpaceX will also attempt to re-land the Falcon 9 first stage on an oceangoing barge for an unprecedented second time, provided there are sufficient fuel reserves remaining after accomplishing its primary mission of delivering SES-10 to GTO, Halliwell stated.

The SES-10 launch comes barely 2 weeks after the prior SpaceX launch of EchoStar XXIII on March 16.

SpaceX, founded by billionaire and CEO Elon Musk, inked a deal in August 2016 with telecommunications giant SES, to refly a ‘Flight-Proven’ Falcon 9 booster.

Luxembourg-based SES and Hawthrone, CA-based SpaceX jointly announced the agreement to “launch SES-10 on a flight-proven Falcon 9 orbital rocket booster.”

The flight proven SpaceX Falcon 9 rocket will deliver SES-10 to a Geostationary Transfer Orbit (GTO).

SES-10 has a launch mass of 5,300 kg or 11,700 pounds, which includes the dry mass and propellant.

The spacecraft utilizes for both chemical propulsion for orbit raising and electric propulsion for station keeping.

SES-10 will replace AMC-3 and AMC-4 to provide enhanced coverage and significant capacity expansion over Latin America, says SES.

“The satellite will be positioned at 67 degrees West, pursuant to an agreement with the Andean Community (Bolivia, Colombia, Ecuador and Peru), and will be used for the Simón Bolivar 2 satellite network.”

Up to 3 additional SES satellites could launch on SpaceX Falcon 9 rockets by the end of this year.

Watch for Kens’ continuing coverage direct from onsite at the Kennedy Space Center press site and Cape Canaveral Air Force Station.

Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.

Ken Kremer

………….

Learn more about SpaceX SES-10, EchoStar 23 and CRS-10 launches to ISS, ULA SBIRS GEO 3 launch, GOES-R launch, Heroes and Legends at KSCVC, OSIRIS-REx, InSight Mars lander, Juno at Jupiter, SpaceX AMOS-6, ISS, ULA Atlas and Delta rockets, Orbital ATK Cygnus, Boeing, Space Taxis, Mars rovers, Orion, SLS, Antares, NASA missions and more at Ken’s upcoming outreach events at Kennedy Space Center Quality Inn, Titusville, FL:

Mar 31, Apr 1: “SpaceX SES-10, EchoStar 23, CRS-10 launch to ISS, ULA Atlas SBIRS GEO 3 launch, GOES-R weather satellite launch, OSIRIS-Rex, SpaceX and Orbital ATK missions to the ISS, Juno at Jupiter, ULA Delta 4 Heavy spy satellite, SLS, Orion, Commercial crew, Curiosity explores Mars, Pluto and more,” Kennedy Space Center Quality Inn, Titusville, FL, evenings

SES CTO Martin Halliway discusses the planned SES-10 telecomsat launch on March 30, 2017 on first ‘flight-proven’ SpaceX Falcon 9 from pad 39A on the Kennedy Space Center, FL. Credit: Ken Kremer/Kenkremer.com

Historic maiden blastoff of SpaceX Falcon 9 rocket from Launch Complex 39A at the Kennedy Space Center) at 9:38 a.m. EDT on Feb 19, 2017, on Dragon CRS-10 resupply mission to the International Space Station (ISS) for NASA. Credit: Ken Kremer/kenkremer.com

The Orbit of Uranus. How Long is a Year on Uranus?

Uranus as seen by NASA's Voyager 2. Credit: NASA/JPL

Uranus is a most unusual planet. Aside from being the seventh planet of our Solar System and the third gas giant, it is also classified sometimes as an “ice giant” (along with Neptune). This is because of its peculiar chemical composition, where water and other volatiles (i.e. ammonia, methane, and other hydrocarbons) in its atmosphere are compressed to the point where they become solid.

In addition to that, it also has a very long orbital period. Basically, it takes Uranus a little over 84 Earth years to complete a single orbit of the Sun. What this means is that a single year on Uranus lasts almost as long as a century here on Earth. On top of that, because of it axial tilt, the planet also experiences extremes of night and day during the course of a year, and some pretty interesting seasonal changes.

Orbital Period:

Uranus orbits the Sun at an average distance (semi-major axis) of 2.875 billion km (1.786 billion mi), ranging from 2.742 billion km (1.7 mi) at perihelion to 3 billion km (1.86 billion mi) at aphelion. Another way to look at it would be to say that it orbits the Sun at an average distance of 19.2184 AU (over 19 times the distance between the Earth and the Sun), and ranges from 18.33 AU to 20.11 AU.

Images of Uranus taken over a four year period using the Hubble Space Telescope. Credit: NASA/ESA/HST

The difference between its minimum and maximum distance from the Sun is 269.3 million km (167.335 mi) or 1.8 AU, which is the most pronounced of any of the Solar Planets (with the possible exception of Pluto). And with an average orbital speed of 6.8 km/s (4.225 mi/s), Uranus has an orbital period equivalent to 84.0205 Earth years. This means that a single year on Uranus lasts as long as 30,688.5 Earth days.

However, since it takes 17 hours 14 minutes 24 seconds for Uranus to rotate once on its axis (a sidereal day). And because of its immense distance from the Sun, a single solar day on Uranus is about the same. This means that a single year on Uranus lasts 42,718 Uranian solar days. And like Venus, Uranus’ rotates in the direction opposite of its orbit around the Sun (a phenomena known as retrograde rotation).

Axial Tilt:

Another interesting thing about Uranus is the extreme inclination of its axis (97.7°). Whereas all of the Solar Planets are tilted on their axes to some degree, Uranus’s extreme tilt means that the planet’s axis of rotation is approximately parallel with the plane of the Solar System. The reason for this is unknown, but it has been theorized that during the formation of the Solar System, an Earth-sized protoplanet collided with Uranus and tilted it onto its side.

A consequence of this is that when Uranus is nearing its solstice, one pole faces the Sun continuously while the other faces away – leading to a very unusual day-night cycle across the planet. At the poles, one will experience 42 Earth years of day followed by 42 years of night.

This is similar to what is experienced in the Arctic Circle and Antarctica. During the winter season near the poles, a single night will last for more than 24 hours (aka. a “Polar Night”) while during the summer, a single day will last longer than 24 hours (a “Polar Day”, or “Midnight Sun”).

Meanwhile, near the time of the equinoxes, the Sun faces Uranus’ equator and gives it a period of day-night cycles that are similar to those seen on most of the other planets. Uranus reached its most recent equinox on December 7th, 2007. During the Voyager 2 probe’s historic flyby in 1986, Uranus’s south pole was pointed almost directly at the Sun.

Seasonal Change:

Uranus’ long orbital period and extreme axial tilt also lead to some extreme seasonal variations in terms of its weather. Determining the full extent of these changes is difficult because astronomers have yet to observe Uranus for a full Uranian year. However, data obtained from the mid-20th century onward has showed regular changes in terms of brightness, temperature and microwave radiation between the solstices and equinoxes.

These changes are believed to be related to visibility in the atmosphere, where the sunlit hemisphere is thought to experience a local thickening of methane clouds which produce strong hazes. Increases in cloud formation have also been observed, with very bright cloud features being spotted in 1999, 2004, and 2005. Changes in wind speed have also been noted that appeared to be related to seasonal increases in temperature.

Uranus Dark Spot
Close up of Uranus Dark Spot, taken by the Hubble Telescope. Credit: NASA/ESA/HST

Uranus’ “Great Dark Spot” and its smaller dark spot are also thought to be related to seasonal changes. Much like Jupiter’s Great Red Spot, this feature is a giant cloud vortex that is created by winds – which in this case are estimated to reach speeds of up to 900 km/h (560 mph). In 2006, researchers at the Space Science Institute and the University of Wisconsin observed a storm that measured 1,700 by 3,000 kilometers (1,100 miles by 1,900 miles).

Interestingly enough, while Uranus’ polar regions receive more energy on average over the course of a year than the equatorial regions, the equatorial regions have been found to be hotter than the poles. The exact cause of this remains unknown, but is certainly believed to be due to something endogenic.

Yep, Uranus is a pretty weird place! On this planet, a single year lasts almost a century, and the seasons are characterized by extreme versions of Polar Nights and Midnight Suns. And of course, an average year brings all kinds of seasonal changes, complete with extreme winds, massive storms, and thickening methane clouds.

We have written many articles about the length of a year on other planets here at Universe Today. Here’s How Long is a Year on the Other Planets?, How Long is a Year on Mercury?, How Long is a Year on Venus?, How Long is a Year on Earth?, How Long is a Year on Mars?, How Long is a Year on Jupiter?, How Long is a Year on Saturn?, How Long is a Year on Neptune? and How Long is a Year on Pluto?

If you’d like more info on Uranus, check out Hubblesite’s News Releases about Uranus. And here’s a link to the NASA’s Solar System Exploration Guide to Uranus.

We have recorded an episode of Astronomy Cast just about Uranus. You can access it here: Episode 62: Uranus.

Sources:

SES ComSat Boss Proclaims High ‘Confidence’ in SpaceX’s Bold 1st ‘Flight-Proven’ Rocket Launch – March 30

The SES-10 satellite was manufactured by Airbus Defence & Space and is based on the Eurostar E3000 platform. It will operate in geostationary orbit.Credit: SES/Airbus

The SES-10 satellite was manufactured by Airbus Defence & Space and is based on the Eurostar E3000 platform. It will operate in geostationary orbit. Credit: SES/Airbus

CAPE CANAVERAL/KENNEDY SPACE CENTER, FL – As the hours tick down to the history making liftoff of the world’s first recycled rocket, the commercial customer SES is proclaiming high “confidence” in the flight worthiness of the “Flight-Proven” SpaceX Falcon 9 booster that will blastoff with a massive Hi-Def TV satellite for telecom giant SES this Thursday, Chief Technology Officer Martin Halliwell told Universe Today at a media briefing.

“We are confident in this booster,” SES CTO Martin Halliwell told me at a press briefing on March 28, regarding SpaceX CEO Elon Musk’s bold vision to slash launch costs by recovering and reusing spent first stage rockets from his firms Falcon 9 launch vehicle.

The milestone SpaceX mission destined to refly the first ever ‘used rocket’ is slated for lift off on Thursday, March 30, at 6:27 p.m. EDT carrying the SES-10 telecommunications payload to orbit atop a ‘Flight-Proven’ Falcon 9 rocket from seaside Launch Complex 39A at NASA’s Kennedy Space Center in Florida.

SES-10 is to be the first ever satellite launching on such a SpaceX flight-proven first stage rocket, Halliwell explained.

The Falcon 9 was designed from the start of development by SpaceX engineers to be reusable.

The nearly six ton satellite will provide significantly improved TV, voice and data service to over 37 million customers in Central and South America.

“This thing is good to go!”

The Falcon 9 booster to be recycled was initially launched in April 2016 for NASA on the SpaceX Dragon CRS-8 resupply mission to the International Space Station (ISS) under contract for the space agency.

Sunset blastoff of SpaceX Falcon 9 carrying SES-9 communications satellite from Space Launch Complex 40 on Cape Canaveral Air Force Station, FL. Credit: Ken Kremer/kenkremer.com

The 156 foot tall first stage was recovered about eight and a half minutes after liftoff via a pinpoint propulsive soft landing on an tiny ocean going droneship prepositioned in the Atlantic Ocean some 400 miles (600 km) off the US East coast.

The SES-10 launch comes barely 2 weeks after the prior SpaceX launch of EchoStar XXIII on March 16.

It also marks the final round of March Launch Madness. Concldung the third and final round of launches this month.

Recovered SpaceX Falcon 9 from Thaicom-8 mission after craning off ‘OCISLY’ droneship to ground processing cradle at Port Canaveral, FL. Workers had removed the first of four landing legs in this view from June 3, 2016. Credit: Ken Kremer/kenkremer.com

The booster is one of eight first stages recovered by SpaceX so far, either by landing on a barge at sea or on a landing pad on the ground.

“We [SES] have been through this vehicle with a fine tooth comb,” Halliwell elaborated.

The boosters are carefully checked and refurbished to confirm their integrity and utility, and the first stage Merlin 1D engines are re-fired multiple times to confirm they will function reliably and robustly.

“SpaceX has been through this booster with a fine tooth comb. This booster is a really good booster.”
Is this a high risk strategy to be first in line launching an expensive satellite on a used rocket, I asked? Why are you confident?

“There is not a huge risk,” Halliwell stated emphatically. “In this particular case we know that the reusability capability is built into the design of the Falcon 9 vehicle. I think its baseline is to fly nine times. We are flight #2.’

“We have tested this thing. We have run the engines up! Halliwell elaborated.

SpaceX has run full duration static fire tests as well as shorter 3 to 5 second hold down tests on the pad.

Indeed this booster was successfully checked out during a brief engine test lasting approximately five seconds at 2 p.m. today, Monday March 27, with the sudden eruption of smoke and ash rushing into the air over historic pad 39A on NASA’s Kennedy Space Center during a picture perfect sunny afternoon – as I witnessed from Space View Park in Titusville, FL.

SpaceX conducts successful static hot fire test of 1st previously flown Falcon 9 booster atop Launch Complex 39A at the Kennedy Space Center on 27 Mar. 2017 as seen from Space View Park, Titusville, FL. History making launch of first recycled rocket is slated for 30 March 2017 with SES-10 telecommunications comsat. Credit: Ken Kremer/Kenkremer.com

“We have also looked at the airframe, Halliwell went on. “We have looked at the various components. This thing is good to go.”

“We don’t believe we are taking an inordinate risk here.”

SpaceX says the cost of a Falcon 9 launch is about $60 million.

Halliwell would not disclose the discount SES is receiving for this launch by utilizing a recycled rocket. But SpaceX officials have been quoted as saying the savings could be between 10 to 30 percent.

“So with that we can go back to our insurers and we can explain that risk exactly. And we can back it up with analysis and test data. So I don’t agree that we are taking a huge risk here!” Halliwell told me.

“From a pricing point of view, the launch cost pricing is really irrelevant. The delta in cost is really not relevant or material.”

The payload was encapsulated inside the payload fairing and bolted on top of the Falcon 9. It will be rolled back out to pad 39A overnight Thursday morning and erected.

13 hours of critical checks are needed to insure the satellite is still functioning perfectly after raising at the pad, Halliwell explained. The timeline is tight to get all the required work done in time to carry out a Thursday evening launch.

Historic maiden blastoff of SpaceX Falcon 9 rocket from Launch Complex 39A at the Kennedy Space Center) at 9:38 a.m. EDT on Feb 19, 2017, on Dragon CRS-10 resupply mission to the International Space Station (ISS) for NASA. Credit: Ken Kremer/kenkremer.com

SpaceX, founded by billionaire and CEO Elon Musk, inked a deal in August 2016 with telecommunications giant SES, to refly a ‘Flight-Proven’ Falcon 9 booster.

Luxembourg-based SES and Hawthrone, CA-based SpaceX jointly announced the agreement to “launch SES-10 on a flight-proven Falcon 9 orbital rocket booster.”

The flight proven SpaceX Falcon 9 rocket will deliver SES-10 to a Geostationary Transfer Orbit (GTO).

SES-10 has a launch mass of 5,300 kg or 11,700 pounds, which includes the dry mass and propellant.

The spacecraft utilizes for both chemical propulsion for orbit raising and electric propulsion for station keeping.

Liftoff of the Falcon 9 carrying the SES-10 telecommunications satellite is now slated for 6:27 p.m. EDT at the opening of the launch window

The two and a half hour launch window closes at 8:57 p.m. EDT.

SpaceX will webcast the launch live.

SpaceX will also attempt to re-land the Falcon 9 first stage for an unprecedented second time, provided there are sufficient fuel reserves remaining after accomplishing its primary mission to delivering SES-10 to GTO, Halliwell stated.

SES-10 will replace AMC-3 and AMC-4 to provide enhanced coverage and significant capacity expansion over Latin America, says SES.

“The satellite will be positioned at 67 degrees West, pursuant to an agreement with the Andean Community (Bolivia, Colombia, Ecuador and Peru), and will be used for the Simón Bolivar 2 satellite network.”

Up to 3 additional SES satellites could launch on SpaceX Falcon 9 rockets by the end of this year.

Stay tuned here for Ken’s continuing Earth and Planetary science and human spaceflight news.

Ken Kremer
………….

Learn more about SpaceX SES-10, EchoStar 23 and CRS-10 launches to ISS, ULA SBIRS GEO 3 launch, GOES-R launch, Heroes and Legends at KSCVC, OSIRIS-REx, InSight Mars lander, Juno at Jupiter, SpaceX AMOS-6, ISS, ULA Atlas and Delta rockets, Orbital ATK Cygnus, Boeing, Space Taxis, Mars rovers, Orion, SLS, Antares, NASA missions and more at Ken’s upcoming outreach events at Kennedy Space Center Quality Inn, Titusville, FL:

Mar 31, Apr 1: “SpaceX SES-10, EchoStar 23, CRS-10 launch to ISS, ULA Atlas SBIRS GEO 3 launch, GOES-R weather satellite launch, OSIRIS-Rex, SpaceX and Orbital ATK missions to the ISS, Juno at Jupiter, ULA Delta 4 Heavy spy satellite, SLS, Orion, Commercial crew, Curiosity explores Mars, Pluto and more,” Kennedy Space Center Quality Inn, Titusville, FL, evenings

Video Caption: SpaceX Falcon 9 hot fire test on March 27, 2017 for SES-10 launch on March 30 on KSC Pad 39A. Credit: Jeff Seibert

Finite Light — Why We Always Look Back In Time

Credit: Bob King

Beads of rainwater on a poplar leaf act like lenses, focusing light and enlarging the leaf’s network of veins. Moving at 186,000 miles per second, light from the leaf arrives at your eye 0.5 nanosecond later. A blink of an eye takes 600,000 times as much time! Credit: Bob King

My attention was focused on beaded water on a poplar leaf. How gemmy and bursting with the morning’s sunlight. I moved closer, removed my glasses and noticed that each drop magnified a little patch of veins that thread and support the leaf.

Focusing the camera lens, I wondered how long it took the drops’ light to reach my eye. Since I was only about six inches away and light travels at 186,000 miles per second or 11.8 inches every billionth of a second (one nanosecond), the travel time amounted to 0.5 nanoseconds. Darn close to simultaneous by human standards but practically forever for positronium hydride, an exotic molecule made of a positron, electron and hydrogen atom. The average lifetime of a PsH molecule is just 0.5 nanoseconds.

Light takes about 35 microseconds to arrive from a transcontinental jet and its contrail. Credit: Bob King

In our everyday life, the light from familiar faces, roadside signs and the waiter whose attention you’re trying to get reaches our eyes in nanoseconds. But if you happen to look up to see the tiny dark shape of a high-flying airplane trailed by the plume of its contrail, the light takes about 35,000 nanoseconds or 35 microseconds to travel the distance. Still not much to piddle about.

The space station orbits the Earth in outer space some 250 miles overhead. During an overhead pass, light from the orbiting science lab fires up your retinas 1.3 milliseconds later. In comparison, a blink of the eye lasts about 300 milliseconds (1/3 of a second) or 230 times longer!

The Lunar Laser Ranging Experiment placed on the Moon by the Apollo 14 astronauts. Observatories beam a laser to the small array, which reflects a bit of the light back. Measuring the time delay yields the Moon’s distance to within about a millimeter. At the Moon’s surface the laser beam spreads out to 4 miles wide and only one photon is reflected back to the telescope every few seconds. Credit: NASA

Light time finally becomes more tangible when we look at the Moon, a wistful 1.3 light seconds away at its average distance of 240,000 miles. To feel how long this is, stare at the Moon at the next opportunity and count out loud: one one thousand one. Retroreflecting devices placed on the lunar surface by the Apollo astronauts are still used by astronomers to determine the moon’s precise distance. They beam a laser at the mirrors and time the round trip.

Venus as a super-thin crescent only 10 hours before conjunction on March 25. The planet was just 2.3 light minutes from the Earth at the time. Credit: Shahrin Ahmad

Of the eight planets, Venus comes closest to Earth, and it does so during inferior conjunction, which coincidentally occurred on March 25. On that date only 26.1 million miles separated the two planets, a distance amounting to 140 seconds or 2.3 minutes — about the time it takes to boil water for tea. Mars, another close-approaching planet, currently stands on nearly the opposite side of the Sun from Earth.

With a current distance of 205 million miles, a radio or TV signal, which are both forms of light, broadcast to the Red Planet would take 18.4 minutes to arrive. Now we can see why engineers pre-program a landing sequence into a Mars’ probe’s computer to safely land it on the planet’s surface. Any command – or change in commands – we might send from Earth would arrive too late. Once a lander settles on the planet and sends back telemetry to communicate its condition, mission control personnel must bite their fingernails for many minutes waiting for light to limp back and bring word.

Before we speed off to more distant planets, let’s consider what would happen if the Sun had a catastrophic malfunction and suddenly ceased to shine. No worries. At least not for 8.3 minutes, the time it takes for light, or the lack of it, to bring the bad news.

Pluto and Charon lie 3.1 billion miles from Earth, a long way for light to travel. We see them as they were more than 4 hours ago.  NASA/JHUAPL/SwRI

Light from Jupiter takes 37 minutes to reach Earth; Pluto and Charon are so remote that a signal from the “double planet” requires 4.6 hours to get here. That’s more than a half-day of work on the job, and we’ve only made it to the Kuiper Belt.

Let’s press on to the nearest star(s), the Alpha Centauri system. If 4.6 hours of light time seemed a long time to wait, how about 4.3 years? If you think hard, you might remember what you were up to just before New Year’s Eve in 2012. About that time, the light arriving tonight from Alpha Centauri left that star and began its earthward journey. To look at the star then is to peer back in time to late 2012.

The Summer Triangle rises fully in the eastern sky around 3 o’clock in the morning in late March. Created with Stellarium

But we barely scrape the surface. Let’s take the Summer Triangle, a figure that will soon come to dominate the eastern sky along with the beautiful summer Milky Way that appears to flow through it. Altair, the southernmost apex of the triangle is nearby, just 16.7 light years from Earth; Vega, the brightest a bit further at 25 and Deneb an incredible 3,200 light years away.

We can relate to the first two stars because the light we see on a given evening isn’t that “old.” Most of us can conjure up an image of our lives and the state of world affairs 16 and 25 years ago. But Deneb is exceptional. Photons departed this distant supergiant (3,200 light years) around the year 1200 B.C. during the Trojan War at the dawn of the Iron Age. That’s some look-back time!

Rho Cassiopeia, currently at magnitude +4.5, is one of the most distant stars visible with the naked eye. Its light requires about 8,200 years to reach our eyes. This star, a variable, is enormous with a radius about 450 times that of the Sun. Credit: IAU/Sky and Telescope (left); Anynobody, CC BY-SA 3.0 / Wikipedia

One of the most distant naked eye stars is Rho Cassiopeiae, yellow variable some 450 times the size of the Sun located 8,200 light years away in the constellation Cassiopeia. Right now, the star is near maximum and easy to see at nightfall in the northwestern sky. Its light whisks us back to the end of the last great ice age at a time and the first cave drawings, more than 4,000 years before the first Egyptian pyramid would be built.

This is the digital message (annotated here) sent by Frank Drake to M13 in 1974 using the Arecibo radio telescope.

On and on it goes: the nearest large galaxy, Andromeda, lies 2.5 million light years from us and for many is the faintest, most distant object visible with the naked eye. To think that looking at the galaxy takes us back to the time our distant ancestors first used simple tools. Light may be the fastest thing in the universe, but these travel times hint at the true enormity of space.

Let’s go a little further. On November 16, 1974 a digital message was beamed from the Arecibo radio telescope in Puerto Rico to the rich star cluster M13 in Hercules 25,000 light years away. The message was created by Dr. Frank Drake, then professor of astronomy at Cornell, and contained basic information about humanity, including our numbering system, our location in the solar system and the composition of DNA, the molecule of life. It consisted of 1,679 binary bits representing ones and zeroes and was our first deliberate communication sent to extraterrestrials. Today the missive is 42 light years away, just barely out the door.

Galaxy GN-z11, shown in the inset, is seen as it was 13.4 billion years in the past, just 400 million years after the big bang, when the universe was only three percent of its current age. The galaxy is ablaze with bright, young, blue stars, but looks red in this image because its light has been stretched to longer spectral wavelengths by the expansion of the universe. Credit: NASA, ESA, P. Oesch, G. Brammer, P. van Dokkum, and G. Illingworth

Let’s end our time machine travels with the most distant object we’ve seen in the universe, a galaxy named GN-z11 in Ursa Major. We see it as it was just 400 million years after the Big Bang (13.4 billion years ago) which translates to a proper distance from Earth of 32 billion light years. The light astronomers captured on their digital sensors left the object before there was an Earth, a Solar System or even a Milky Way galaxy!

Thanks to light’s finite speed we can’t help but always see things as they were. You might wonder if there’s any way to see something right now without waiting for the light to get here? There’s just one way, and that’s to be light itself.

From the perspective of a photon or light particle, which travels at the speed of light, distance and time completely fall away. Everything happens instantaneously and travel time to anywhere, everywhere is zero seconds. In essence, the whole universe becomes a point. Crazy and paradoxical as this sounds, the theory of relativity allows it because an object traveling at the speed of light experiences infinite time dilation and infinite space contraction.

Just something to think about the next time you meet another’s eyes in conversation. Or look up at the stars.

Watch Rotating Horns of Venus at Dawn

Venus inferior conjunction
Venus, just 10.5 hours before inferior conjunction on March 25th. Image credit and copyright: Shahrin Ahmad (@Shahgazer)

Venus inferior conjunction
Venus just 10.5 hours before inferior conjunction on March 25th. Image credit and copyright: Shahrin Ahmad (@Shahgazer)

Have you seen it yet? An old friend greeted us on an early morning run yesterday as we could easily spy brilliant Venus in the dawn, just three days after inferior conjunction this past Saturday on March 25th.

This was an especially wide pass, as the planet crossed just over eight degrees (that’s 16 Full Moon diameters!) north of the Sun. We once managed to see Venus with the unaided eye on the very day of inferior conjunction back in 1998 from the high northern latitudes of the Chena Flood Channel just outside of Fairbanks, Alaska.

The planet was a slender 59.4” wide, 1% illuminated crescent during this past weekend’s passage, and the wide pass spurred many advanced imagers to hunt for the slim crescent in the daytime sky. Of course, such a feat is challenging near the dazzling daytime Sun. Safely blocking the Sun out of view and being able to precisely point your equipment is key in this endeavor. A deep blue, high contrast sky helps, as well. Still, many Universe Today readers rose to the challenge of chronicling the horns of the slender crescent Venus as they rotated ’round the limb and the nearby world moved once again from being a dusk to dawn object.

Venus rotating horns
A daily sequence showing the ‘Horns of Venus’ rotate as it approaches inferior conjunction. Image credit and copyright: Shahrin Ahmad (@ShahGazer)

The orbit of Venus is tilted 3.4 degrees with respect to the Earth, otherwise, we’d get a transit of the planet like we did on June 5-6th, 2012 once about every 584 days, instead of having to wait again until next century on December 10th, 2117.

The joint NASA/European Space Agency’s SOlar Heliospheric Observatory (SOHO) mission also spied the planet this past weekend as it just grazed the 15 degree wide field of view of its Sun-observing LASCO C3 camera:

Venus SOHO
The glow of Venus (arrowed) just barely bleeding over into the field of view of SOHO’s LASCO C3 camera. Credit: SOHO/NASA/LASCO

Venus kicks off April as a 58” wide, 3% illuminated crescent and ends the month at 37” wide, fattening up to 28% illumination. On closest approach, the planet presents the largest apparent planetary disk possible as seen from the Earth. Can you see the horns? They’re readily readily apparent even in a low power pair of hunting binoculars. The coming week is a great time to try and see a crescent Venus… with the naked eye. Such an observation is notoriously difficult, and right on the edge of possibility for those with keen eyesight.

One problem for seasoned observers is that we know beforehand that (spoiler alert) that the Horns of Venus, like the Moon, always point away from the direction of the Sun.

True Story: a five year old girl at a public star party once asked me “why does that ‘star’ look like a tiny Moon” (!) This was prior to looking at the planet through a telescope. Children generally have sharper eyes than adults, as the lenses of our corneas wear down and yellow from ultraviolet light exposure over the years.

Still, there are tantalizing historical records that suggest that ancient cultures such as the Babylonians knew something of the true crescent nature of Venus in pre-telescopic times as well.

The Babylonian frieze of Kudurru Melishipak on display at the Louvre, depicting the Sun Moon and Venus. According to some interpretations, the goddess Ishtar (Venus) is also associated with a crescent symbol… possibly lending credence to the assertion that ancient Babylonian astronomers knew something of the phases of the planet from direct observation. Credit: Wikimedia Commons/Image in the Public Domain.

Another fun challenge in the coming months is attempting to see Venus in the daytime. This is surprisingly easy, once you know exactly where to look for it. A nearby crescent Moon is handy, as occurs on April 23rd, May 22nd, and June 20th.

Daytime Venus
Venus (arrowed) near the daytime Moon. Photo by author.

Strangely enough, the Moon is actually darker than dazzling Venus in terms of surface albedo. The ghostly daytime Moon is just larger and easier to spot. Many historical ‘UFO’ sightings such as a ‘dazzling light seen near the daytime Moon’ by the startled residents of Saint-Denis, France on the morning on January 13th, 1589 were, in fact, said brilliant planet.

The Moon near Venus on May 22nd. Credit: Stellarium.

Venus can appear startlingly bright to even a seasoned observer. We’ve seen the planet rise as a shimmering ember against a deep dark twilight sky from high northern latitudes. Air traffic controllers have tried in vain to ‘hail’ Venus on more than one occasion, and India once nearly traded shots with China along its northern border in 2012, mistaking a bright conjunction of Jupiter and Venus for spy drones.

The third brightest object in the sky behind the Sun and the Moon, Venus is even bright enough to cast a shadow as seen from a dark sky site, something that can be more readily recorded photographically.

Watch our nearest planetary neighbor long enough, and it will nearly repeat the same pattern for a given apparition. This is known as the eight year cycle of Venus, and stems from the fact that 13 Venusian orbits (8x 224.8 days) very nearly equals eight Earth years.

Follow Venus through the dawn in 2017, and it will eventually form a right triangle with the Earth and the Sun on June 3rd, reaching what is known as greatest elongation. This can vary from 47.2 to 45.4 degrees from the Sun, and this year reaches 45.9 degrees elongation in June. The planet then reaches half phase known as dichotomy around this date, though observed versus theoretical dichotomy can vary by three days. The cause of this phenomenon is thought to be the refraction of light in Venus’ dense atmosphere, coupled with observer bias due to the brilliance of Venus itself. When do you see it?

Also, keep an eye out for the ghostly glow on the night-side of Venus, known as Ashen Light. Long thought to be another trick of the eye, there’s good evidence to suggest that this long reported effect actually has a physical basis, though Venus has no large reflecting moon nearby… how could this be? The leading candidate is now thought to be air-glow radiating from the cooling nighttime side of the planet.

Cloud enshrouded Venus held on to its secrets, right up until the Space Age less than a century ago… some observers theorized that the nighttime glow on Venus was due to aurorae, volcanoes or even light pollution from Venusian cities (!). This also fueled spurious sightings of the alleged Venusian moon Neith right up through the 19th century.

Venus should also put in a showing 34 degrees west of the Sun shining at magnitude -4 during the August 21st, 2017 total solar eclipse. Follow that planet, as it makes a complex meet up with Mars, Mercury, and the Moon in late September of this year.

More to come!

-Read about planets, occultations, comets and more for the year in our 101 Astronomical Events for 2017, out as a free e-book from Universe Today.