“Engineering helped create a world in which no injustice could be hidden,” the retired NASA astronaut (now deceased) said in that speech, explaining that engineering is more focused on envisioning possibilities than the facts-based science professions.
While Armstrong makes no direct reference to his historic 1969 moon landing in the speech, the animation is peppered with references including the famous “bootprint” picture taken by his crewmate, Buzz Aldrin.
We’d be interested in knowing what scientists or science fans think of his point of view. Is Armstrong’s view too limited for science, or an accurate description? Watch the video, and let us know in the comments.
Extreme ultraviolet light streams out of an X-class solar flare as seen in this image captured on March 29, 2014, by NASA's Solar Dynamics Observatory. This image blends two wavelengths of light: 304 and 171 Angstroms, which help scientists observe the lower levels of the sun's atmosphere. Image Credit: NASA/SDO.
If you sit at a fairly high latitude, you may want to keep an eye out your window Tuesday (April 1) and Wednesday. A powerful X-1 class flare erupted from the sun on Saturday (March 29), sparking an active space weather forecast from the National Oceanic and Atmospheric Administration.
The solar flare erupted from sunspot AR2017 and happened to be aimed at the right direction to bring material to Earth. The associated coronal mass ejections (CMEs) will send streams of particles towards our planet, which could get pulled towards the poles and cause light shows as they interact with molecules in the upper atmosphere.
“NOAA forecasters estimate a 35 percent to 60 percent chance of polar geomagnetic storms on April 1-2 when at least three CMEs are expected to deliver glancing blows to Earth’s magnetic field,” SpaceWeather.com wrote. “The best-guess forecast calls for minor G1-class storms. High-latitude sky watchers should be alert for auroras.”
Aurora seen near Fairbanks, Alaska on March 21, 2014. Credit and copyright: John Chumack.
At the top of this story, you can view a video of the flare from the Solar Dynamics Observatory, a NASA satellite launched in 2010 to observe the sun’s activity. This not only has applications for aurora watchers, but also for those people concerned about the effect CMEs have on Earth’s satellites, power lines and other sensitive infrastructure.
Below is an older picture from the Solar and Heliospheric Observatory, a joint NASA and European Space Agency mission that also keeps an eye on solar activity. The sun has an 11-year cycle of solar activity, and you can see peak year 2001 at the front of the image along with quieter years 1996 and 2006 near the back. The year 2014 is just off the peak for this solar cycle.
A solar cycle in X-rays. The peak in 2001 is visible at the front, with quietest years 1996 and 2006 near the back. The sun’s 11-year-solar cycle sees an increase in sunspots and solar activity at its peak. The year 2014 is close to the peak year for activity, but the cycle has been more muted than the 2001 cycle. Credit: Steele Hill, SOHO, NASA/ESA
Our own Sun produces flares, but we are protected by our magnetosphere, and by the distance from the Sun to Earth. Credit: NASA/ Solar Dynamics Observatory,
When will the next big solar flare occur? How much damage could it cause to power lines and satellites? These are important questions for those looking to protect our infrastructure, but there’s still a lot we need to figure out concerning space weather.
The video above, however, shows magnetic lines weaving together from the surface of the Sun in 2012, eventually creating an eruption that was 35 times our planet’s size and sending out a surge of energy. It’s these energetic flares that can hit Earth’s atmosphere and cause auroras and power surges.
While models of this have been made before, this is the first time the phenomenon was caught in action. Scientists saw it using NASA’s Solar Dynamics Observatory.
Models of the flares show they typically occur amid distorted magnetic fields, the University of Cambridge noted, showing that the lines can “reconnect while slipping and flipping around each other.” Before the flare happens, the magnetic field lines line up in an arc across the sun’s surface (photosphere). That phenonemon is called field line footprints.
“In a smooth, non-entangled arc the magnetic energy levels are low, but entanglement will occur naturally as the footpoints move about each other,” the release added. “Their movement is caused as they are jostled from below by powerful convection currents rising and falling beneath the photosphere. As the movement continues, the entanglement of field lines causes magnetic energy to build up.”
When the energy gets to great, the lines let go of the energy, creating the solar flare and coronal mass ejection that can send material streaming away from the sun. A note, this observation was made of an X-class flare — the strongest kind of flare — and scientists say they are not sure if this phenomenon is true of all kinds of flares. That said, the phenomenon would be harder to spot in smaller flares.
You can read more about the research in the Astrophysical Journal or in preprint version on Arxiv. It was led by Jaroslav Dudik, a researcher at the University of Cambridge’s center for mathemetical sciences.
An extra-tropical cyclone seen off the coast of Japan, March 10, 2014, by the GPM Microwave Imager. The colors show the rain rate: red areas indicate heavy rainfall, while yellow and blue indicate less intense rainfall. The upper left blue areas indicate falling snow. Credit: NASA/JAXA
KENNEDY SPACE CENTER, FL – Weather researchers worldwide now have the ability to capture unprecedented three-dimensional images and detailed rainfall measurements of cyclones, hurricanes and other storms from space on a global basis thanks to the newest Earth observing weather satellite – jointly developed by the US and Japan.
NASA and the Japan Aerospace Exploration Agency (JAXA) have now released the first images captured by their Global Precipitation Measurement (GPM) Core Observatory satellite.
GPM soared to space on Feb. 27, exactly one month ago, during a spectacular night launch from the Japanese spaceport at the Tanegashima Space Center on Tanegashima Island off southern Japan.
The newly released series of images show precipitation falling inside a vast extra-tropical cyclone cascading over a vast swath of the northwest Pacific Ocean, approximately 1,000 miles off the coast of eastern Japan.
3D view inside an extra-tropical cyclone observed off the coast of Japan, March 10, 2014, by GPM’s Dual-frequency Precipitation Radar. The vertical cross-section approx. 4.4 mi (7 km) high show rain rates: red areas indicate heavy rainfall while yellow and blue indicate less intense rainfall. Credit: JAXA/NASA
“It was really exciting to see this high-quality GPM data for the first time,” said GPM project scientist Gail Skofronick-Jackson at NASA’s Goddard Spaceflight Center in Greenbelt, Md., in a NASA statement.
“I knew we had entered a new era in measuring precipitation from space. We now can measure global precipitation of all types, from light drizzle to heavy downpours to falling snow.”
The imagery was derived from measurements gathered by GPM’s two advanced instruments: JAXA’s high resolution dual-frequency precipitation (DPR) radar instrument (Ku and Ka band), which imaged a three-dimensional cross-section of the storm, and the GPM microwave imager (GMI) built by Ball Aerospace in the US which observed precipitation across a broad swath.
“The GMI instrument has 13 channels that measure natural energy radiated by Earth’s surface and also by precipitation itself. Liquid raindrops and ice particles affect the microwave energy differently, so each channel is sensitive to a different precipitation type,” according to a NASA statement.
On March 10, 2014 the Global Precipitation Measurement (GPM) Core Observatory passed over an extra-tropical cyclone about 1,055 miles (1,700 km) east of Japan’s Honshu Island. Formed when a cold air mass wrapped around a warm air mass near Okinawa on March 8, it moved NE drawing cold air over Japan before weakening over the North Pacific. Credit: NASA/JAXA
The 3850 kilogram GPM observatory is the first satellite designed to measure light rainfall and snow from space, in addition to heavy tropical rainfall.
The data were released following check out and activation of the satellites pair of instruments.
“GPM’s precipitation measurements will look like a CAT scan,” Dr. Dalia Kirschbaum, GPM research scientist, told me during a prelaunch interview with the GPM satellite in the cleanroom at NASA’s Goddard Space Flight Center in Greenbelt, Md.
“The radar can scan through clouds to create a three dimensional view of a clouds structure and evolution.”
The $933 Million GPM observatory will provide high resolution global measurements of rain and snow every 3 hours. It is a joint venture between NASA and JAXA.
It will collect a treasure trove of data enabling the most comprehensive measurements ever of global precipitation – and across a wide swath of the planet where virtually all of humanity lives from 65 N to 65 S latitudes.
The GMI instrument has 13 channels, each sensitive to different types of precipitation. Channels for heavy rain, mixed rain and snow, and snowfall are displayed of the extra-tropical cyclone observed March 10, off the coast of Japan. Multiple channels capture the full range of precipitation. Credit: NASA/JAXA
GPM orbits at an altitude of 253 miles (407 kilometers) above Earth – quite similar to the International Space Station (ISS).
GPM is the lead observatory of a constellation of nine highly advanced Earth orbiting weather research satellites contributed by the US, Japan, Europe and India.
NASA’s next generation Global Precipitation Measurement (GPM) observatory inside the clean room at NASA Goddard Space Flight Center, MD. Technicians at work on final processing during exclusive up-close inspection tour by Universe Today. GPM launched on February 27, 2014 and will provide global measurements of rain and snow every 3 hours. Credit: Ken Kremer/kenkremer.com
Stay tuned here for Ken’s continuing GPM, Curiosity, Opportunity, Chang’e-3, SpaceX, Orbital Sciences, LADEE, MAVEN, MOM, Mars and more planetary and human spaceflight news.
Learn more at Ken’s upcoming presentations at the NEAF convention on April 12/13 and at Washington Crossing State Park, NJ on April 6. Also at the Quality Inn Kennedy Space Center, Titusville, FL, March 29.
The Expedition 39/40 crew just before climbing into their Soyuz spacecraft in Kazakhstan on March 25, 2014. From top, Oleg Artemyev (Roscosmos), Steve Swanson (NASA) and Alexander Skvortsov (Roscosmos). Credit: NASA/Joel Kowsky
Update, 8:33 p.m. EDT: The Soyuz spacecraft arrived safely at station at 7:53 p.m. EDT (11:53 a.m. UTC) and coverage of the hatch opening is scheduled at 10:15 p.m. EDT (2:15 a.m. UTC).
After spending an extra couple of days in the cramped Russian Soyuz spacecraft, the incoming International Space Station crew will likely be very be glad to get out and stretch their legs. You can check out the festivities live in the video link above.
Three people are set to make a docking with the orbiting complex at 7:58 p.m. EDT (11:58 p.m. UTC). If all goes to schedule, they’ll pop the hatch open at 10:40 p.m. EDT (2:40 a.m. UTC). Meanwhile, engineers are trying to figure out what caused the malfunction that prevented a docking as planned on Tuesday (March 25).
Remember that all schedules are subject to change, so tune into NASA TV well before each event happens.
The Expedition 39/40 crew lifted off Tuesday afternoon (EDT) from Kazakhstan to take a fast track to the space station that should have seen them dock on launch day. The Soyuz has to make three engine firings or burns to accomplish this. The docking was cancelled after the third burn did not happen as planned. The Russian Federal Space Agency (Roscosmos) has determined this was because the spacecraft was in the wrong orientation, but the underlying cause is still being investigated.
Once this happened, the crew switched to a standard backup procedure to bring them to the station in two days instead. (This path, in fact, was what all crews did up until last year.) The crew is safe and in good spirits heading up to the docking, NASA has said. The Soyuz has done several other engine firings since, with no incident.
The Soyuz crew includes Steve Swanson (NASA), Alexander Skvortsov (Roscosmos) and Oleg Artemyev (Roscosmos). Awaiting them on the station are Koichi Wakata (Japan Aerospace Exploration Agency), Rick Mastracchio (NASA) and Mikhail Tyurin (Roscosmos). Wakata is in command of the station, marking a first for Japan’s astronaut corps.
The Expedition 39/40 crew gives a thumbs-up during quarantine prior to their March 25, 2014 launch from Kazakhstan. From left: Steve Swanson (NASA), Alexander Skvortsov (Roscosmos) and Oleg Artemyev (Roscosmos). Credit: NASA
Despite a problem that held up last night’s International Space Station docking, the Expedition 39/40 crew is doing well as they execute a standard backup procedure to bring their Soyuz spacecraft to the station on Thursday, NASA said.
The crew was originally expected to dock with the station around 11 p.m. EDT (3 a.m. UTC), but an error with the spacecraft’s position in space prevented the engines from doing a third planned “burn” or firing to make that possible, NASA said in an update.
“At this point, the crew is in good shape and the vehicle appears to be in good shape,” said Kenny Todd, the space station’s operations integration manager, in an interview on NASA TV Wednesday morning (EDT). “At this point, everything looks real good.”
In fact, the spacecraft has done a couple of burns since to get it into the right spot for a docking Thursday evening, Todd added. (So it appears the crew just missed the window to get there on Tuesday night.) The underlying cause of the orientation problem was not mentioned in the interview, presumably because it’s still being investigated.
NASA is quite familiar with a two-day route to the space station as up until last year, all crews took two days to get to the space station. This took place for 14 years until a rapider method of reaching the orbiting complex within hours was introduced.
The crew includes Steve Swanson (NASA), Alexander Skvortsov (Roscosmos) and Oleg Artemyev (Roscosmos), who will join three people already on station when they arrive.
Japanese astronaut Koichi Wakata plays around wiith humanoid robot Robonaut 2 during Expedition 39 in March 2014. Credit: NASA
Current station residents Koichi Wakata (the commander, of the Japan Aerospace Exploration Agency), Rick Mastracchio (NASA) and Mikhail Tyurin (Roscosmos) got to sleep in this morning and had some minor modifications to their schedule because of the docking delay, Todd added.
Instead of taking the day off as planned, the crew will do some work. A planned ISS software update for last night is going to be pushed “down the line”, Todd said, adding that the forthcoming SpaceX launch on Sunday and docking on Tuesday is still going ahead as planned.
We’ll provide more updates as the situation progresses. Docking is scheduled for 7:58 p.m. EDT (11:58 p.m. UTC) Thursday and will be covered on NASA Television.
The launch of Expedition 39/40's Steve Swanson, Alexander Skvortsov and Oleg Artemyev as seen from space. Picture captured by NASA's Rick Mastracchio aboard the International Space Station on March 25, 2014. Credit: Rick Mastracchio
Seriously, how cool is this picture? The International Space Station crew caught an incredible view of their three future crewmates rocketing up to meet them today around 5:17 p.m. EDT (9:17 p.m. UTC).
Expedition 39’s Rick Mastracchio (from NASA) shared this on Twitter, casually mentioning that he will expect more crewmates to arrive later today. Upon the rocket were Steve Swanson (NASA), Alexander Skvortsov (Roscosmos) and Oleg Artemyev (Roscosmos).
Check out the launch video and some NASA pictures of the activities below the jump. (Update, 10:21 p.m. EDT: One of the engine firings did not take place as planned, meaning the astronauts will not dock with the station as planned tonight. The crew is safe and doing a standard backup plan that will bring them to the station on Thursday. We will provide updates as the situation progresses.)
Three models of NASA's Z-2 suit unveiled to the public in March 2014 for people to vote on their favorite design. From left, "Biomimicry", "Technology" and "Trends In Society." Click for a larger version. Credit: NASA (Photo combination: Elizabeth Howell)
If you ever wanted to participate in spacesuit design, even in a small way, here’s your big chance. NASA is asking the public to choose which design of the futuristic Z-2 “planetary mobility” suit prototype will be used by astronauts while evaluating how well the spacesuit works.
There are three options (which you can see above), and NASA promises the winning design will be used in pool training at NASA’s Neutral Buoyancy Laboratory, the Johnson Space Center “rockyard” to simulate Mars exploration, and in vacuum tests. Outer space is not an option because of “micrometeorite, thermal and radiation protection” considerations, however.
In NASA’s words, here’s a quick summary of the prototypes:
Biomimicry: The “Biomimicry” design draws from an environment with many parallels to the harshness of space: the world’s oceans. Mirroring the bioluminescent qualities of aquatic creatures found at incredible depths, and the scaly skin of fish and reptiles found across the globe, this design reflects the qualities that protect some of Earth’s toughest creatures.
Technology: “Technology” pays homage to spacesuit achievements of the past while incorporating subtle elements of the future. By using Luminex wire and light-emitting patches, this design puts a new spin on spacewalking standards such as ways to identify crew members.
Trends In Society: “Trends in Society” is based off of just that: being reflective of what every day clothes may look like in the not too distant future. This suit uses electroluminescent wire and a bright color scheme to mimic the appearance of sportswear and the emerging world of wearable technologies.
The Z-2 includes several improvements over its Z-1 predecessor, which won an invention award from Time magazine in 2012. These include a “hard composite” upper torso that is intended to be more durable, better shoulder and hip joints, and boots that would be more useful on a planet.
An astronaut retrieves a sample from an asteroid in this artist's conception. Credit: NASA
Got some ideas about how to snag an asteroid? NASA has just announced $6 million in opportunities for its asteroid retrieval initiative, which would see astronauts explore one of these space rocks in the 2020s if the agency receives budgetary approval to go through with the idea.
First proposed in the 2014 fiscal year budget (which has yet to be approved by Congress), the agency is moving forward with the idea by getting ideas from industry about the best way to approach the asteroid, capture it, and other priority areas. Up to 25 proposals will be selected.
The announcement comes just ahead of a one-day conference to (in part) gather public ideas for the mission. For those who weren’t able to snag one of the sold-out seats, NASA is offering virtual attendance at the forum. Follow the instructions at this page and then make a note of the program schedule on Wednesday.
In NASA’s words, these are the topics that are priority areas for solicitation:
Asteroid capture system concepts including using deployable structures and autonomous robotic manipulators;
Rendezvous sensors that can be used for a wide range of mission applications including automated rendezvous and docking and asteroid characterization and proximity operations;
Commercial spacecraft design, manufacture, and test capabilities that could be adapted for development of the Asteroid Redirect Vehicle (ARV);
Studies of potential future partnership opportunities for secondary payloads on either the ARV or the SLS;
Studies of potential future partnership opportunities for the Asteroid Redirect Crewed Mission, or other future missions, in areas such as advancing science and in-situ resource utilization, enabling commercial activities, and enhancing U.S. exploration activities in cis-lunar space after the first crewed mission to an asteroid.
“NASA is developing two mission concepts for the Asteroid Redirect Mission (ARM): one concept uses a robotic spacecraft to capture a whole small near-Earth asteroid, and the second concept uses largely the same robotic spacecraft to capture a cohesive mass from a larger asteroid,” the agency added in the solicitation documents.
Artist’s conception of NASA’s asteroid retrieval mission. Credit: NASA
“In both mission concepts, the asteroid mass would be redirected into a stable orbit around the Moon. Astronauts aboard the Orion spacecraft launched on the Space Launch System (SLS) would rendezvous with the captured asteroid mass in lunar orbit and collect samples for return to Earth.”
The agency is framing this initiative as a way to prepare for longer-duration missions (such as going to Mars) as well as better characterizing the threat from asteroids — which is certainly on many people’s minds after a meteor broke up over Chelyabinsk, Russia just over a year ago.
Expedition 10 commander Leroy Chiao is reflected in a water sphere on board the International Space Station in 2004. Credit: NASA
“Here on board the ISS, we turn yesterday’s coffee into tomorrow’s coffee” is a slogan that sounds a little like a Don Draper-led advertising campaign. Seriously, though, it’s a nifty way in which Expedition 39 commander Koichi Wakata describes in this video (also embedded below) how the astronauts drink purified urine on the station.
The water is perfectly hygienic once it runs through the system, and moreover, it could be a useful trick for future space colonists to remember.
Water is heavy, at about 8.3 pounds per gallon (or roughly 1 kg/liter) at room temperature. And astronauts in space do need to go through a lot of it to prevent dehydration and other illnesses. Throw in demanding activities such as exercising two hours a day or going on a spacewalk, and you can see how quickly people in space go through it.
Everything sent into space has an associated launch cost with it, and space engineers are always looking for ways to shave a few grams here or there. By installing the water purification system (which was completed in 2009 with Wakata on board), NASA said it would be able to reduce the amount sent up to station.
When people speak of space colonies on the Moon or Mars, they often talk about landing them near a large source of water ice and then using that to help support the people working there. As NASA once wrote in a worksheet, “Until an orbiting grocery store is opened, recycling of water and air will be crucial for crew survival.”
Check out Wakata’s explanation of the water recycling system below. For more information on recycling water in Mars colonies, one source to start with could be T. A. Heppenheimer’s “Colonies In Space”, published on the National Space Society website.
