Posted on by Ken Kremer

3 Days to Red Planet Touchdown – Watch the Harrowing Video of Car-Sized Curiosity Careening to Crater Floor


Video Caption: This 11-minute animation depicts key events of how NASA’s Mars Science Laboratory mission will land the huge rover Curiosity on Mars on August 5/6, 2012. Credit: NASA

Well, here we are 3 days from the thrilling ‘touchdown’ of Curiosity on Mars on the boldest mission yet by humans to the Red Planet – Seeking Signs of Life beyond Earth!

The Curiosity Mars Science Lab rover is by far the hardest and most complex robotic mission that NASA has ever attempted. She marks a quantum leap beyond anything tried before in terms of the technology required to land this 2000 pound beast and the science she’ll carry out for a minimum 2 year prime mission.

So watch this harrowing video (above) – Outlining how Curiosity slams into the Martian atmosphere at 13200 MPH and comes to rest at 0 MPH after surviving the “7 Minutes of Terror” with an unprecedented guided entry, rocket powered descent, neck snapping supersonic parachute deployment and never before used Sky Crane maneuver – and be sure you’re safely seated !

The car-sized Curiosity has entered the final 72 hours of careening towards a crater floor on Mars.

After the nail biting entry, descent and landing (EDL), the 6 wheeled rover Curiosity is scheduled to touchdown inside Gale Crater at about 1:31 a.m. EDT (531 GMT) early on Aug. 6 (10:31 p.m. PDT on Aug. 5).

“It looks a little crazy !” said Adam Steltzner, MSL Entry, Descent and Landing Lead engineer JPL , at today’s (Aug. 2) pre-landing briefing for reporters at NASA’s Jet Propulsion Lab (JPL) in Pasadena, Calif. “But it’s the least crazy compared to other methods we evaluated.”

“Everything looks good for Sunday night. Over 300 Years of human individual contributions went into the MSL EDL system. We pull 10 Earth G’s or more of acceleration during first contact with the Martian atmosphere.”

See the detailed EDL graphic below –
Image caption: Entry, Descent and Landing (EDL) Timeline – click to enlarge for full image. Credit: NASA

Curiosity is the first mobile soil and rock sampling and chemistry lab dispatched to Mars. It’s also the first astrobiology mission to Mars since the twin Viking missions of the 1970’s.

“We are about to land a small compact car on Mars with a trunk load of instruments. It’s an amazing feat, exciting and daring. It’s fantastic,” said Doug McCuistion, director of the Mars Exploration Program at NASA Headquarters at the JPL briefing.

“It’s an extreme pleasure to be here. MSL has a huge reach, to the past, the future and around the world. Since the heatshield is nearly the size of the Orion heat shield, we’ll also learn an enormous amount about how we’ll land humans on Mars.”

“MSL is a workhorse for the future,” McCuistion emphasized.

Curiosity will search for the ingredients of life in the form of organic molecules – the carbon based molecules which are the building blocks of life as we know it. The one-ton behemoth is packed to the gills with 10 state-of-the-art science instruments including a 7 foot long robotic arm, scoop, drill and laser rock zapper.

Watch NASA TV online for live coverage of the Curiosity landing on Aug 5/6:
mars.jpl.nasa.gov or www.nasa.gov

Ken Kremer

Posted on by Nancy Atkinson

HiRISE Camera to Attempt Imaging Curiosity’s Descent to Mars

Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (HiRISE) camera captured this image of Phoenix hanging from its parachute as it descended to the Martian surface. Credit: NASA/JPL/University of Arizona.

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Note: This article was updated on Aug. 3 with additional information.

The HiRISE camera crew on the Mars Reconnaissance Orbiter will attempt an audacious repeat performance of the image above, where the team was able to capture an amazing shot of the Phoenix lander descending on a parachute to land on Mars’ north polar region. Only this time it will try to focus on the Mars Science Laboratory’s Curiosity rover descending to touch down in Gale Crater. It will be all or nothing for the HiRISE team, as they get only one shot at taking what would likely be one of the most memorable images of the entire mission for MRO.

“We’re only making one attempt on MSL here,” Christian Schaller of the HiRISE team told Universe Today. “The EDL (Entry, Descent and Landing) image is set up so that as MSL is descending, MRO will be slewing the HiRISE field of view across the expected descent path. The plan is to capture MSL during the parachute phase of descent.”

Schaller is the software developer responsible for the primary planning tools the MRO and HiRISE targeting specialists and science team members use to plan their images.

Last December, when Universe Today learned of this probable imaging attempt, HiRISE Principal Investigator Alfred McEwen confirmed for us that, indeed, the team was working to make it happen. The preferred shot would be to “capture the rover hanging from the skycrane, but the timing may be difficult,” McEwen said.

It would take an impeccable – and fortuitous – sense of timing to get that shot, but since MSL’s EDL won’t happen on a precisely exact timetable, the HiRISE team will take their one shot and see what happens.

“We’ve been gradually updating the exact timing of the sequence over the past couple of weeks as the MSL navigation team, the MRO navigation team and the MRO flight engineering team refines that descent path and MRO slew,” Schaller said via email, “and we think we’ve pretty much got it nailed down at this point. I think it’s a real testament to NASA and its partners that we can even think about doing this.”

HiRISE will actually be taking two images, but the first is a “throwaway” warmup image taken about 50 minutes prior to MSL’s descent, designed to heat the camera’s electronics up to the preferred temperature for getting good image data.

“The warmup image we’re taking is a long-exposure throwaway that we’re taking on the night side of Mars,” Schaller explained. “It’s a 5,000 microsecond per line exposure, compared to a more typical 100 microsecond per line exposure during normal surface imaging. These warmup data will be useless, and we don’t even bother sending them back to Earth; we just dump them from the MRO filesystem once the exposure is complete.”

Schaller said the warmup image starts executing at 04:17 UTC/9:17 PM PDT. The real image starts executing at 05:09 UTC/10:09 PM PDT, centered on 10:16 PM as the time MSL and MRO navigation teams have determined MSL will pass through HiRISE’s field of view.

This image will be an approximately 500 microseconds per line exposure, to match the MRO’s slew rate.


Caption: Artist impression of MRO orbiting Mars. Credit: NASA

UPDATE (Aug. 3): In checking with McEwen, he said that Mars Express and Odyssey are NOT planning to image the descent, but they are supporting EDL via UHF relay, and the plans to use CTX has been dropped.

“HiRISE plans are to definitely attempt the image, unless there is a late upset to the MRO spacecraft,” McEwen said via email on August 3. “The engineers estimate we have a 60% chance of capturing MSL in our image.”

MRO’s Context Camera (CTX) will also be attempting to image Curiosity’s descent, as will NASA’s Mars Odyssey and ESA’s Mars Express and all the spacecraft have been performing special maneuvers to be aligned in just the right place – nearby to MSL’s point of entry into Mars’ atmosphere.

While Odyssey and Mars Express’ cameras may not have the resolving power to capture MSL itself, the powerful HiRISE camera does. However, it has a narrower field of view, so as much skill and planning as this requires, the team will need a little luck, too. But there’s also the CTX.

“CTX has a much larger field of view and will likely capture it,” McEwen said, “but at 20X lower resolution than HiRISE, which should still be good enough to detect the parachute.”

For those concerned about the fuel required for all these orbiters to reposition themselves just to take a few pictures, the expenditure is nothing that isn’t required anyway. All the spacecraft need to be in position to support MSL during the critical EDL event, and the images are pure extra-benefit, if not an incredible exercise for the imaging teams.

So while we’ll all be crossing our fingers for a successful landing for Curiosity, I’m on my way to find a rabbit’s foot or 4-leaf clover for HiRISE.

Posted on by Nancy Atkinson

Data from Black Hole’s Edge Provides New Test of Relativity

From a NASA press release:

Last year, astronomers discovered a quiescent black hole in a distant galaxy that erupted after shredding and consuming a passing star. Now researchers have identified a distinctive X-ray signal observed in the days following the outburst that comes from matter on the verge of falling into the black hole.

This tell-tale signal, called a quasi-periodic oscillation or QPO, is a characteristic feature of the accretion disks that often surround the most compact objects in the universe — white dwarf stars, neutron stars and black holes. QPOs have been seen in many stellar-mass black holes, and there is tantalizing evidence for them in a few black holes that may have middleweight masses between 100 and 100,000 times the sun’s.

Until the new finding, QPOs had been detected around only one supermassive black hole — the type containing millions of solar masses and located at the centers of galaxies. That object is the Seyfert-type galaxy REJ 1034+396, which at a distance of 576 million light-years lies relatively nearby.

“This discovery extends our reach to the innermost edge of a black hole located billions of light-years away, which is really amazing. This gives us an opportunity to explore the nature of black holes and test Einstein’s relativity at a time when the universe was very different than it is today,” said Rubens Reis, an Einstein Postdoctoral Fellow at the University of Michigan in Ann Arbor. Reis led the team that uncovered the QPO signal using data from the orbiting Suzaku and XMM-Newton X-ray telescopes, a finding described in a paper published today in Science Express.

The X-ray source known as Swift J1644+57 — after its astronomical coordinates in the constellation Draco — was discovered on March 28, 2011, by NASA’s Swift satellite. It was originally assumed to be a more common type of outburst called a gamma-ray burst, but its gradual fade-out matched nothing that had been seen before. Astronomers soon converged on the idea that what they were seeing was the aftermath of a truly extraordinary event — the awakening of a distant galaxy’s dormant black hole as it shredded and gobbled up a passing star. The galaxy is so far away that light from the event had to travel 3.9 billion years before reaching Earth.

Video info: On March 28, 2011, NASA’s Swift detected intense X-ray flares thought to be caused by a black hole devouring a star. In one model, illustrated here, a sun-like star on an eccentric orbit plunges too close to its galaxy’s central black hole. About half of the star’s mass feeds an accretion disk around the black hole, which in turn powers a particle jet that beams radiation toward Earth. Credit: NASA’s Goddard Space Flight Center/Conceptual Image Lab

The star experienced intense tides as it reached its closest point to the black hole and was quickly torn apart. Some of its gas fell toward the black hole and formed a disk around it. The innermost part of this disk was rapidly heated to temperatures of millions of degrees, hot enough to emit X-rays. At the same time, through processes still not fully understood, oppositely directed jets perpendicular to the disk formed near the black hole. These jets blasted matter outward at velocities greater than 90 percent the speed of light along the black hole’s spin axis. One of these jets just happened to point straight at Earth.

Nine days after the outburst, Reis, Strohmayer and their colleagues observed Swift J1644+57 using Suzaku, an X-ray satellite operated by the Japan Aerospace Exploration Agency with NASA participation. About ten days later, they then began a longer monitoring campaign using the European Space Agency’s XMM-Newton observatory.

“Because matter in the jet was moving so fast and was angled nearly into our line of sight, the effects of relativity boosted its X-ray signal enough that we could catch the QPO, which otherwise would be difficult to detect at so great a distance,” said Tod Strohmayer, an astrophysicist and co-author of the study at NASA’s Goddard Space Flight Center in Greenbelt, Md.

As hot gas in the innermost disk spirals toward a black hole, it reaches a point astronomers refer to as the innermost stable circular orbit (ISCO). Any closer to the black hole and gas rapidly plunges into the event horizon, the point of no return. The inward spiraling gas tends to pile up around the ISCO, where it becomes tremendously heated and radiates a flood of X-rays. The brightness of these X-rays varies in a pattern that repeats at a nearly regular interval, creating the QPO signal.

The data show that Swift J1644+57’s QPO cycled every 3.5 minutes, which places its source region between 2.2 and 5.8 million miles (4 to 9.3 million km) from the center of the black hole, the exact distance depending on how fast the black hole is rotating. To put this in perspective, the maximum distance is only about 6 times the diameter of our sun. The distance from the QPO region to the event horizon also depends on rotation speed, but for a black hole spinning at the maximum rate theory allows, the horizon is just inside the ISCO.

“QPOs send us information from the very brim of the black hole, which is where the effects of relativity become most extreme,” Reis said. “The ability to gain insight into these processes over such a vast distance is a truly beautiful result and holds great promise.”

Read our previous article on Swift J1644+57

Lead image caption: This illustration highlights the principal features of Swift J1644+57 and summarizes what astronomers have discovered about it. Credit: NASA’s Goddard Space Flight Center

Posted on by Nancy Atkinson

Reminiscent of Apollo, Australian Facilities Will Receive First Signals of Curiosity Rover Landing

The movie “The Dish” tells the wonderful story of how Australian radio communication dishes saved the day as Apollo 11 landed on the Moon, allowing the world to watch in wonder. While the movie isn’t entirely accurate, Australia does have a marvelous history of providing tracking and communication with spacecraft on historic missions. The tradition continues with the upcoming landing of the Mars Science Laboratory Curiosity rover when it sets down on Mars on August 5/6 after a nail-biting entry, descent and landing.

The Canberra Deep Space Communication Complex (CDSCC) will be the main tracking station for the landing activities. Its 70-m and two 34-m antennas will receive signals from the spacecraft both directly and then relayed through another NASA spacecraft, Mars Odyssey, in orbit around the Red Planet.

The 64-m Parkes telescope – the one featured in “The Dish” — will record signals directly from the spacecraft as a backup in case there is a problem with the relaying. But as the spacecraft descends, it will drop below the Martian horizon (and out of direct sight of Earth-based antennas) about two minutes before touchdown, and Parkes will cease receiving its signals.

A third, smaller, antenna managed by the European Space Agency (ESA) at New Norcia near Perth in WA will provide extra redundancy. It will receive signals from the spacecraft recorded and re-sent through ESA’s Mars Express satellite, which is in orbit around Mars.

Signals from the Canberra station will be sent directly to mission scientists at NASA’s Jet Propulsion Laboratory (JPL) in Pasadena, California. Data from Parkes and New Norcia will be sent later for analysis.

While the landing is not controlled from Earth, as the lag-time in radio signals (13.8 minutes one way) makes any input from Earth impossible, tracking the spacecraft as it approaches Mars is very important.

Astrophoto: Tracking Curiosity by Glen James Nagle
Tracking Curiosity. Image Credit: Glen James Nagle

“We are looking forward to receiving and sending that touchdown signal from MSL, so we can help end those ‘7 minutes of terror’ for the amazing scientists and engineers waiting at JPL,” said Glen Nagle, Education and Public Outreach Officer at Canberra Deep Space Communication Complex, via email. Nagle took this panoramic image, above, early in December 2011 in Canberra while the dishes were getting their first data from MSL after its launch, so the facility has been an integral part of guiding the spacecraft during its entire journey to Mars.

The last opportunity to send the spacecraft any commands will be two hours before it enters the atmosphere. “After that, it’s on its own,” said Nagle.

NASA engineers also want to know exactly where the spacecraft enters the atmosphere so they can locate the rover when it lands, and of course, the hopeful rover fans back on Earth will want to find out as soon as possible to know if the landing succeeded or not.

The spacecraft will slam into the atmosphere at 20,000 km per hour. Over the next seven minutes the craft and then its payload must be slowed to essentially zero.

The landing has several stages: cruise, deployment of the entry capsule and then the parachute, separation of the heat shield, and finally the operation of the “skycrane” that will lower the 900-kg rover, Curiosity, onto the Martian surface.

As each stage is successfully completed the spacecraft will send a unique tone indicating that it has occurred.

During the landing, the mission scientists can only watch and wait. They call this time the “seven minutes of terror”.

The exact landing time for the spacecraft is determined by several factors, including descent time on the parachute, Martian winds, and any variation how the spacecraft flies under power before the landing. Confirmation of a touchdown signal could be received on Earth at 05:31 UTC on Aug. 6 (10:31 p.m. PDT on Aug. 5 and 1:31 a.m. EDT Aug. 6, 3.31 pm AEST Aug. 6) plus or minus a minute.

Winds could mean that descent time on the parachute is longer, but at this time of year on Mars the weather is very stable and is not expected to cause any problems.

If the final set of tones is not heard, Mars Odyssey will listen for them again when it orbits over the landing site 1.5 hours later.

“The expertise of Australian personnel in space communications and CSIRO’s partnership with NASA will be showcased during this critical event in the Mars Science Laboratory’s mission,” says Chief of CSIRO Astronomy and Space Science, Dr. Phil Diamond. “All of our technology and our people are ready.”

And so are all the rover fans back on Earth!

Read more about what it has taken to navigate MSL all the way to Mars at our previous article, “How Will MSL Navigate to Mars? Very Precisely.”

And here’s another previous article about how we *really* watched the footage from the Apollo 11 Moon landing, thanks to the Australian radio dishes.

Lead image caption: The 70-m antenna at the Canberra Deep Space Communication Complex. (Credit: CDSCC)

source: CSIRO

Posted on by Nancy Atkinson

Take a Virtual Visit to Kennedy Space Center Via Google Maps

A view of space shuttle Atlantis using Street View in Google Maps.

From experience, I can attest to what an amazing experience it is to be at Kennedy Space Center, home of where NASA launches many of its spacecraft. But if you can’t get there in person, you can now take a virtual trip – and see many views the public can’t normally see – thanks to a new partnership between KSC and Google Maps Street View. Using the interactive 360-degree views from the Street View, you can take a walk through the cavernous Vehicle Assembly Building or stand at the top of Launch Pad 39A.

See the video below for a sneak peak into the experience:

Google Maps with Street View lets you explore Kennedy’s facilities, roads and structures. You can see the history of spaceflight by viewing the Apollo/Saturn V Center, Space Shuttle Main Engine shop, Orbiter Processing Facility-3, the Launch Control Center, the Space Station Processing Facility and the center’s iconic Vehicle Assembly Building.

The new maps also allows virtual visitors to check in at KSC and watch as it transitions to the multipurpose launch complex of the future, revamping existing infrastructure and facilities to provide the flexibility to host a variety of commercial and government spacecraft, rockets and other craft.

Users may go directly to Google Maps, search for “NASA Shuttle Landing Facility,” and drag the orange “pegman” icon on the left-hand side to an area outlined in blue. From there, users can navigate around the area by moving up and down pathways and looking around in 360 degrees. The entire collection of images also is available in the Google Street View gallery:

http://www.google.com/streetview

The new partnership is part of KSC’s 50th anniversary celebration. For more information about Kennedy’s 50th anniversary, visit:

http://go.nasa.gov/y0VdRi

For more information about Kennedy, visit:

http://www.nasa.gov/kennedy

Posted on by Nancy Atkinson

Comedian Stephen Colbert Talks with NASA’s John Grunsfeld About Curiosity Rover Landing


The Colbert Report Mon – Thurs 11:30pm / 10:30c
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NASA Chief Scientist John Grunsfeld took Stephen Colbert’s “Colbert Report” audience on a guided tour through the seven minutes of terror that the Curiosity rover will endure to land on Mars, and the two also discussed the possibility of life on Mars. Grunsfeld also shocked Colbert for a moment when he said the Curiosity rover won’t discover a thing … but then continued to say it will be the scientists who make the discoveries, and Grunsfeld predicted it will be an amazing 2 years for the MSL scientists during Curiosity’s prime mission.
Continue reading “Comedian Stephen Colbert Talks with NASA’s John Grunsfeld About Curiosity Rover Landing”

Posted on by Nancy Atkinson

Progress Resupply Ship Takes Fast-Track to ISS, Arriving 6 Hours After Launch

After a flawless launch, an unmanned Russian Progress resupply ship used a new expedited technique to reach the International Space Station in hours instead of days. Progress 48 was loaded with almost three tons of food, fuel and supplies for the six crew members, and it docked successfully to the Pirs docking compartment on August 1, just six hours after the launch from the Baikonur Cosmodrome in Kazakhstan at 19:35 UTC (3:35 p.m. EDT, 1:35 a.m. Aug. 2 Baikonur time). The fast trip and rendezvous was designed to test a method for conducting additional firings of the Progress engines early in its mission to expedite the time required for a Russian vehicle to reach the complex.

Russian officials say the technique could be applied to manned Soyuz vehicles in the future to improve crew comfort and extend the life of the Soyuz return vehicle.

Russian cosmonaut Gennady Padalka has been quoted as saying it is every cosmonaut’s dream to only have a 6-hour flight in the cramped Soyuz!

Russian engineers and managers are still assessing the new technique, but by all appearances the quick trip seemed to be a great success. This Progress vehicle will stay at the ISS until December.

During the docking, NASA also tested a new technique of attitude control for the ISS which will save fuel, requiring 10 times less fuel to put the station in the proper orientation relative to Earth for the unpiloted cargo vehicle’s arrival.

According to Pooja Jesrani, lead attitude determination and control officer (ADCO) for this expedition at the Mission Control Center in Houston, the new maneuver is called the optimal propellant maneuver, or OPM. OPM is an improvement on the standard zero propellant maneuver, or ZPM, also developed by Draper Laboratory. The OPM takes into account the need to make the orientation, or attitude, changes to the space station faster than the ZPM. This speed avoids thermal concerns on the exterior of the station’s modules.

“Maneuvers such as the OPM will increase the International Space Station’s efficiency by using less propellant,” Jesrani said. “Additionally, the reduction in thruster firings during an OPM results in the station enduring lower structural loads. These benefits, among others, will help increase the longevity of the station.”

The maneuvers to and from the docking attitude are expected to save more than 90 percent of the fuel typically used when a Russian cargo spacecraft docks with the orbiting outpost.

Source: NASA

Posted on by Jenny Winder

CINEMA and the Cube-Shaped Future of Space Science

Caption: Jerry Kim, a former student and systems engineer, holds the CINEMA nanosatellite before it was packaged up and sent to NASA in January 2012. Credit: Robert Sanders.

We all will be biting our nails on August 5th as Curiosity makes its perilous descent to the surface of Mars. We have put all our eggs in the biggest, heaviest, most expensive basket, with one of the the most complex science packages and landing procedures. But there is another mission that launches this Friday that likes to keep things small, simple, cheap and accessible!

Scheduled to launch Friday, Aug. 3 from Space Launch Complex-3 at Vandenberg Air Force Base, at 12:27 a.m. PDT CINEMA (CubeSat for Ions, Neutrals, Electrons, & MAgnetic fields) is only one of 11 tiny cubesat satellites that are hitching a lift on an Atlas V rocket alongside the main payload, classified satellite
NROL-36.

ESA included seven Cubesats in the payload for Vega’s maiden flight back in February, but this will be the first time for NASA. Cubesats are modular, cheap, nanosatellites, measuring 10 cm per side, with a maximum mass of 1 kg. CINEMA is comprised of three such cubes, forming a shoebox-sized package weighing 3.15 kg and was developed by students at the University of California, Berkeley, Kyung Hee University in Korea, Imperial College London, Inter-American University of Puerto Rico, and University of Puerto Rico, Mayaguez.

CINEMA is designed to obtain images of the electrical ring current that encircles the Earth and which, during large magnetic storms can knock out our power grids. It carries the STEIN (Suprathermal Electrons, Ions, and Neutrons) Sensor, which will produce an image of the high-energy charged particles in Earth’s atmosphere, mostly ionized hydrogen and oxygen, by detecting energetic neutral atoms (ENAs) As ionized particles spiral around magnetic field lines surrounding Earth, they occasionally hit a neutral particle and grab an electron, transforming into ENAs that travel in a straight line. These can reveal the energy and location of the charged particles from which they came. CINEMA will be joined next year by three identical satellites, two launched by Korea and another by NASA, together they will monitor the 3-dimensional structure of the ring current. Also on board is the MAGIC (MAGnetometer from Imperial College) instrument, provided by Imperial College London, to measure changes in Earth’s magnetic field caused by magnetic storms.

CINEMA is only one of five university-built CubeSats aboard the Atlas V rocket. As they can be bought for only around $1,000 and can then fitted with sensors, transmitters, cameras etc, being able to include multiple satellites in a single launch keeps costs down. Universities can use cubesats to give students hands-on experience of designing, planning, building, running and monitoring a real scientific space mission.

CINEMA principal investigator Robert Lin, professor emeritus of physics and former director of UC Berkeley’s Space Sciences Laboratory, explained some of the pros and cons of cubesats. “There is more risk with these projects, because we use off-the-shelf products, 90 percent of the work is done by students, and the parts are not radiation-hard,” he said. “But it is cheaper and has the latest hardware. I will be very impressed if it lasts more than a year in orbit.”

Additionally, being small means that these satellites pose no threat as space junk either, burning up harmlessly in Earth’s atmosphere when they reach the end of their lifespan.

Find out more about CINEMA at the UC Berkley News Center

Posted on by Ken Kremer

4 Days to Mars: Curiosity activates Entry, Descent and Landing Timeline – EDL Infographic

It’s 4 Days to Mars – and NASA’s Curiosity Mars Science Lab (MSL) spacecraft is now flying under the control of the crafts autonomous entry, descent and landing timeline and picking up speed as she plunges ever faster to the Red Planet and her Rendezvous with Destiny.

“Timeline activated. Bleep-bop. I’m running entry, descent & landing flight software all on my own. Countdown to Mars: 5 days,” Curiosity tweeted Tuesday night.

See below an EDL explanatory infographic timeline outlining the critical sequence of events which must unfold perfectly for Curiosity to safely survive the “7 Minutes of Terror” set to begin on the evening of August 5/6.

Aug. 1 TV Viewing Alert – 11:30 PM EDT – see NASA Science Chief John Grunsfeld tonight (Wed, Aug. 1) on the Colbert Report


Image Caption: Curiosity EDL infographic – – click to enlarge

And the excitement is building rapidly for NASA’s biggest, boldest mission ever to the Red Planet as the flight team continues to monitor Curiosity’s onboard systems and flight trajectory. Yesterday, the flight team successfully carried out a memory test on the software for the mechanical assembly that controls MSL’s descent motor, configured the spacecraft for its transition to entry, descent and landing approach mode, and they enabled the spacecraft’s hardware pyrotechnic devices.

Curiosity remains healthy and on course. If fine tuning for the targeted landing ellipse is needed, the next chance to fire on board thrusters to adjust the trajectory is Friday, Aug. 3.

The 4th of 6 possible Trajectory Correction Maneuver (TCM) firings was just accomplished on Sunday, July 29 – details here.

The car sized Curiosity rover is scheduled to touchdown on Mars at about 1:31 a.m. EDT (531 GMT) early on Aug. 6 (10:31 p.m. PDT on Aug. 5) inside Gale Crater and next to a 3 mile (5 km) mountain taller that the tallest in the US.

Gale Crater is 154 km (96 mi) in diameter and dominated by a layered mountain rising some 5 km (3 mi) above the crater floor which exhibits exposures of minerals that may have preserved evidence of past or present Martian life.

Curiosity is packed with 10 state-of-the-art science experiments that will search for organic molecules and clay minerals, potential markers for signs of Martian microbial life and habitable zones.

Watch NASA TV online for live coverage of the Curiosity landing on Aug 5/6:
mars.jpl.nasa.gov or www.nasa.gov

Ken Kremer

Posted on by Elizabeth Howell

Google’s 5 Most Memorable Space Doodles

Google’s one of those tech companies that makes a big deal about space exploration.

There’s not only the Google Lunar X-Prize, or its maps of the Moon and Mars, or memorable April Fool’s pranks such as the lunar Google Copernicus Hosting Environment and Experiment in Search Engineering (G.C.H.E.E.S.E.)

The Mountain View, Calif.-based search giant often puts space front and center in its periodic “Google Doodles”, which are variations of its logo shown on the site. Google’s been pencilling those since 1998. Over the years the sketches have become more elaborate – and sometimes animated!

After reviewing the space doodles featured on Google’s Doodle site, here are five of the most memorable of them:

May 1-5, 2000 – Google Aliens series

 

This appears to be the first set of space-themed Google Doodles. The drawings are simple – for the most part, they show a UFO flying past or landing on the Google logo. Still, running them in a series over several days was smart, as it encouraged Internet users to visit the young search engine several days in a row to see what was happening next. More eyes on the page is always good for advertising.

Jan. 15, 2004 – Spirit lands on Mars

Mars landings are always big media events, and NASA was in the midst of a bonanza of attention in 2004 as both Spirit and Opportunity successfully touched down on the Red Planet. Thousands of Google users would have been searching out the rovers’ latest exploits. Commemorating Spirit’s landing in a doodle, just as that excitement was at a fever pitch, was a great way for Google to highlight the ability for users to seek out information about the rovers on its own site.

Aug. 9, 2010 – Anniversary of Belka and Stelka spaceflight

The best Google Doodles are those that show you what you don’t know before. In this case, few outside the space community are likely aware of who Belka and Stelka were, and where their spaceflight fits in history. (They were among a series of animal flights flown in the 1960s to determine the risks of space travel to humans.) From Google’s perspective, running a doodle one needs to learn more about encourages users to click on it, generating more page views.

June 15, 2011 – Total lunar eclipse, featuring Slooh

This is a brilliant example of cross-promotion. Astronomy geeks are well-aware of Slooh, a site that turns telescopes to celestial events such as the recent Venus transit of the sun. Google brought the site to the masses through promoting Slooh’s June 15, 2011 lunar eclipse feed right on the home page; the colour of the moon in the logo changed as the eclipse progressed. Google also showed the eclipse on its YouTube channel and on Google Earth, and promoted the Slooh Android app (also hosted by Google.) Slooh mentioned Google’s participation on its own website, too.

Nov. 8, 2011 – Edmond Halley’s birthday

Commemorating Edmond Halley’s birthday is not unique in itself, as Google has singled out other astronomers for the honour – see Ruby Payne-Scott and Johann Gottfried Galle, for example. What makes this sketch memorable is you can barely see the “Google” logo in the doodle. This is a company that is so confident in its brand that it is willing to let its readers fill in the blanks by imagination. (Astute readers will notice Scott’s doodle follows the same principle, but Halley’s doodle did run first.)

What other doodles should Universe Today readers check out? Share your thoughts in the comments.

All images are from Google’s Doodle website.

Elizabeth Howell (M.Sc. Space Studies ’12) is a contributing editor for SpaceRef and award-winning space freelance journalist living in Ottawa, Canada. Her work has appeared in publications such as SPACE.com, Air & Space Smithsonian, Physics Today, the Globe and Mail, the Canadian Broadcasting Corp.,  CTV and the Ottawa Business Journal.