dimanche 13 décembre 2015

Russian military satellite successfully launches by Proton-M rocket









Russian Ministry of  Defense emblem.

December 13, 2015

(Illustration) Proton-M launch

Russia’s Proton-M launched on its seventh flight of the year Sunday morning, beginning a lengthy mission to deploy a Garpun military communications satellite. The rocket departed Baikonur at 06:19 local time (00:19 UTC) to begin a nine-hour journey to geostationary orbit that resulted in a successful deployment of the satellite.

Launch of Kosmos Garpun Satellite (Illustration video, launch of  20 sept. 2011)

Garpun, meaning Harpoon, is a series of new-generation space-to-ground communications satellites dedicated to support Russia’s military space assets.

Garpun military communications satellite

The Garpun constellation, like its predecessor, is designed to provide data relay capabilities for Russia’s fleet of reconnaissance satellites, such as the Persona electro-optical imaging spacecraft and Lotos-S signals intelligence vehicles. It fulfils the same function for Russia as the National Reconnaissance Office’s Quasar – or Satellite Data System (SDS) – satellites do for the United States.

Images, Video, Text, Credits: ROSCOSMOS/ISS Reshetnev/NASA Spaceflight.com/William Graham.

Greetings, Orbiter.ch

vendredi 11 décembre 2015

Zenit Rocket successfully launches Electro-L №2 from the Baikonur Cosmodrome












ROSCOSMOS logo.

11/12/2015


December 11, 2015 at 16:45 MSK (Moscow Time) from Launch Complex 45 area Baikonur Cosmodrome, successful launch vehicle (LV) "Zenit-2SB" with the upper stage (RB) "Fregat-SB" and meteorological spacecraft (SC) "Electro-L" №2. The successful launch carried out from specialists and enterprises of Roscosmos space industry of Russia.

After liftoff of the launcher "Zenith", the separation of the upper stage passed normally.

Liftoff (LV) Zenit-2SB with (SC) Electro-L number 2

The spacecraft "Electro-L" №2 is a meteorological remote sensing device that will provide multispectral imaging the entire disk of the Earth in visible and infrared light.

MCC began to administer the hydro-meteorological satellite "Electro-L" №2

Mission Control Center (MCC) began to administer the spacecraft "Electro-L" №2. The launch took place on December 11, 2015 at 16:45 MSK from the Baikonur Cosmodrome using a launch vehicle "Zenit-2SB" with the upper stage "Fregat-SB".

Propulsion launcher worked in normal mode, and the spacecraft "Electro-L" №2 launched into Earth orbit reference. Satellite flight control personnel carried Lead Operational Control Team, consisting of specialists from the PMU and representatives of developers of the spacecraft.

"Electro-L" №2, which developer is FSUE NPO. SA Lavochkin, - the second in a series of weather satellites and heliogeophysical destination. It is designed for use in geostationary hydrometeorological space system (GGKS) "Electro".

"Electro-L" №2 satellite

Appointment GGKS - ensuring operational information relevant services for analysis and forecast weather on a global scale; study the state of the seas and oceans, the conditions for the flight aviation heliogeophysical situation in near-Earth space, the state of the ionosphere and the Earth's magnetic field, as well as - for the monitoring of climate and global change, monitoring of emergencies and environmental monitoring.

Currently, MCC manages the spacecraft scientific and socio-economic purpose. Including satellites opto-electronic monitoring "Resurs-DK1", "Resource-P" №1 and №2, hydrometeorological spacecraft "Electro-L" №1 and №2, "Canopus-B" №1, as well as satellites Space systems relay information "Luch-5A", "Luch-5B" and "Luch-5B".

ROSCOSMOS Press Releases:

http://www.federalspace.ru/21880/

http://www.federalspace.ru/21881/

Images, Video, Text, Credits: ROSCOSMOS/Translation: Orbiter.ch Aerospace/Roland Berga.

Best regards, Orbiter.ch

Saving NASA's STEREO-B: The 189-million-mile Road to Recovery












NASA - STEREO Mission logo.

Dec. 11, 2015

On Oct. 1, 2014, NASA mission operations lost communication with one of the two spacecraft of the Solar and Terrestrial Relations Observatory, or STEREO, mission, just as the spacecraft was about to orbit around the other side of the sun. Though they haven’t heard from the Behind spacecraft, also known as STEREO-B, in over a year, the spacecraft has finally emerged into a region where it can once again receive radio signals. Scientists have a plan to get it back—and their chances only get better with time.

The two STEREO spacecraft, launched in October 2006, were originally designed to complete a two-year mission, ending in 2008. But—like many NASA spacecraft—they lasted much longer. The long lives of the two STEREO spacecraft, now nine years old, have been a boon for scientists studying the sun and its influence throughout the solar system. The two STEREOs slowly drifted away from Earth as they orbited the sun, one ahead and one behind our home planet, giving scientists constantly-improving views of the sun’s far side, allowing us for the first time to see the whole sun at once. 

However, there are always challenges associated with operating a spacecraft for more than four times its original lifespan. In STEREO’s case, its orbit was the biggest hurdle. The same slow drift that lets the two STEREO spacecraft give us widely varying views of the sun means that each spacecraft eventually lay on the other side of the sun from Earth, leading to a three-month period where communication was impossible due to the sun’s interference.


Image above: The lines of communication to both STEREO spacecraft—Ahead in red and Behind in blue—are now far enough from the sun that mission operators can send signals to both spacecraft. STEREO-A is in communication and operating normally, and mission operators have resumed attempts to contact STEREO-B following an October 2014 loss of communications. Image Credits: NASA/Goddard Space Flight Center Scientific Visualization Studio.

“The sun emits strongly in nearly every wavelength, making it the biggest source of noise in the sky,” said Dan Ossing, mission operations manager for the STEREO mission at the Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland. “Most deep space missions only have to deal with sun interference for a day or so, but for each of the STEREO spacecraft, this period lasted nearly four months.”

When the team realized that the STEREO spacecraft would operate long enough to enter this interference zone, they began planning.

“We had to take a spacecraft that was meant to talk to Earth every day and get it ready for over three months of radio silence,” said Ossing.

The STEREO spacecraft were designed with a command loss timer, an automatic reset button that restarts the spacecraft after 72 hours without contact. This reset is intended to correct any issues that could be preventing communication. The command loss timer can’t be changed—meaning that during its phase on the other side of the sun the two STEREO spacecraft would be rebooting every three days for over three months straight.

Regardless, mission operators planned to make it work. They were in the middle of testing the reset by intentionally withholding communications from STEREO-B for three days—a test that had already been completed with great success on STEREO-A—when communications were lost.

The hard reset happened as expected, 72 hours and 20 minutes after operators stopped communications with the spacecraft. After the reset, STEREO-B was supposed to power itself back on, identify certain stars so it could point its antenna at Earth, and send down a status report.

At first, everything went well. Seconds after the reset, the STEREO team received a signal from STEREO-B—but it was much weaker than they expected, and it quickly faded away. That was the last time we heard from STEREO-B.

The signal received was so weak and so brief that the team was able to extract only a few packets of data to form a partial status report. From that small amount of information, the STEREO team was able to extrapolate the most likely case for where the Behind spacecraft is and what it’s doing.


Animation above: STEREO-B captured this view of an erupting coronal mass ejection on July 23, 2012. The unique vantage points of the two STEREO spacecraft gave us unprecedented simultaneous views of the entire sun. Animation Credits: NASA/STEREO.

“The telemetry showed that the Inertial Measurement Unit, or IMU—which tells the spacecraft if and how fast it’s rotating—failed in a way we didn’t expect,” said Ossing. “Rather than cutting out altogether, it was feeding incorrect information into the guidance and control computer.”

The STEREO team thinks this bad information led the guidance and control computer down a path that eventually sent the spacecraft spinning, leaving its solar panels dark most of the time and its battery only intermittently charged.

If STEREO-B had stayed in contact, this is the kind of problem the STEREO team could fix. Though not easy, it’s a matter of instructing STEREO-B’s computer to ignore the information from that particular IMU. However, contact with STEREO-B cut out before the team could correct the error, meaning that the spacecraft is drifting in space with incorrect information about how it’s moving—a big problem for a spacecraft that needs to keep itself pointed at the sun to stay powered on.

“The bad IMU told STEREO-B that it was spinning, even though it was stationary,” said Ossing. “The spacecraft would have automatically taken steps to correct the supposed spin.”

The problem? STEREO-B’s methods for stopping a spin—including spinning internal reaction wheels and firing its thrusters—would cause a stationary spacecraft to start spinning. And based on the STEREO team’s simulation of what the spacecraft would have done, it’s likely now spinning in a way that means its solar panels are getting sunlight only part of the time, leaving it without power for long periods.

“When STEREO-B’s gets enough power to start booting up, there are several systems that come on automatically,” said Bill Thompson, chief observer for the STEREO mission at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “But those systems are probably draining all the power and preventing the battery from charging up. We need the battery to have a decent charge before the transmitter can be turned on and send us a signal.”

As of Nov. 30, 2015, spacecraft operators have had three three-hour blocks of time on the Deep Space Network each week to try and contact STEREO-B. The first two blocks are dedicated to building up the charge in the spacecraft’s battery by telling it turn off the flight systems that boot up automatically. If STEREO-B can reduce the amount of power it consumes during those brief periods when its battery is charging, the spacecraft could remain on long enough to talk to—and receive commands from—Earth. The third block in each sequence is spent sending commands to turn on the spacecraft’s transmitter.

“If it’s not transmitting, we have no way of knowing if our efforts are working,” said Ossing.

The transmitter requires a command to turn on after a charge-up because of its enormous power. If the transmitter were automatic, it could have turned on while the spacecraft was still being built and tested here on Earth or during launch, posing a danger to people on the ground.

Artist's view of the STEREO spacecraft. Image Credit: NASA

Though spacecraft operators have an initial plan to make contact with STEREO-B, the path to recovery isn’t clear or easy. Part of the problem is how little information we have about what caused the loss of communications with STEREO-B.

“The only concrete information we have is that the IMU was feeding bad information to the guidance and control system,” said Ossing. “From there, we made educated guesses about what the spacecraft would do.”

Part of the problem is uncertainty about STEREO-B’s position—since it has been drifting out of contact for over a year, mission operators don’t know exactly where it is. Further complicating this is the likelihood that STEREO-B would have used its thrusters as part of its effort to correct the nonexistent spin, possibly pushing it even further off course. This means that the STEREO team will have to sweep their signal over a significant portion of sky to make sure they reach STEREO-B.

NASA has recovered spacecraft from similar situations before—notably, ESA/NASA’s Solar and Heliospheric Observatory, or SOHO, was out of contact for six weeks in 1998 before it was recovered. But the distance to SOHO was much smaller, only about a million miles, compared to the 189-million-mile gap between Earth and STEREO-B.

As with all spacecraft, we don’t know exactly what frequency STEREO-B will be listening for. Typically, operators will sweep through the range of frequencies that the spacecraft’s receiver can pick up until the spacecraft locks on to one, a process that usually takes a minute or two. But this is impractical for STEREO-B, given the huge distance, which yields a round-trip communications delay of over half an hour.

“The Deep Space Network was able to create an acquisition technique that can sweep through a frequency segment in about ten seconds,” said Ossing. “We’ve tested it on the Ahead spacecraft, and it worked even better than expected.”

Furthermore, the distance means that any signal that has a hope of reaching STEREO-B must be much, much stronger than the signals we send to near-Earth missions. Engineers have a plan to increase the power of the signal we send to STEREO-B through something called constructive interference. By combining the signals from multiple stations in the Deep Space Network with specific timing and configurations, the waves that form the radio signals collide perfectly to create an even stronger signal.

“Constructive interference creates a new signal that’s more powerful than the sum of its parts,” said Thompson. “We’re combining signals from three 34-meter antennas, which will give us a signal more than twice as powerful as a 70-meter antenna.” 

Because STEREO-B is so far from Earth, any signal it sends back to us will likely be too weak for the Deep Space Network to interpret. So, several of the largest radio telescopes in the world—including the Green Bank Radio Telescope, Arecibo Observatory, and the Allen Telescope Array—will be listening for STEREO-B’s transmission.

The STEREO-B recovery will be fraught with challenges—but it will only get easier over time. Because the spacecraft is on an orbit similar to Earth’s, but lagging behind, Earth will lap STEREO-B in 2023, meaning that the spacecraft gets closer to us every day that passes until then.

“In 2019, the spacecraft will be far enough from the sun that we could image it directly with Hubble and figure out the rate of spin,” said Ossing. “We’re very hopeful that we’ll recover STEREO-B, but it’s just going to take time.”

STEREO is the third mission in NASA's Solar Terrestrial Probes program, which is managed by NASA Goddard for NASA’s Science Mission Directorate, in Washington, D.C.

Related Links:

- STEREO-A Resumes Normal Operations: http://www.nasa.gov/feature/goddard/nasa-s-stereo-a-resumes-normal-operations

- NASA's STEREO mission website: http://www.nasa.gov/stereo

Images (mentioned), Animation (mentioned), Text, Credits: NASA’s Goddard Space Flight Center/Sarah Frazier/Rob Garner.

Greetings, Orbiter.ch

Ride along with Rosetta through the eyes of OSIRIS












ESA - Rosetta Mission patch.

11 December 2015

Rosetta’s OSIRIS camera team has launched a new website to showcase their recent images of Comet 67P/Churyumov–Gerasimenko.

The high-resolution images, taken either with the narrow- or wide-angle scientific imaging camera, will show the comet as recently as the day before.

They will be posted to a dedicated website but followers can also subscribe to a mailing list to receive the images directly via email.

The cadence of the images released will depend on the scientific operations of the spacecraft and in particular on the as-run OSIRIS observations on any given day, along with the availability of images downloaded from the spacecraft.

A minimum of an image per week should be expected, up to an image a day if they are taken daily.

Comet on 10 December 2015 from OSIRIS narrow-angle camera

“Following perihelion and a far excursion, we are now back at closer distances – about 100 km – to the comet, providing a view similar to that when we first arrived on 6 August 2014,” says Holger Sierks, principal investigator for the camera at the Max Planck Institute for Solar System Research in Göttingen, Germany.

“We’d like to share this view with the community and the general public, in near-real time, as we re-approach and eventually descend to the surface of the comet.”

The images will be released by a robotic system in JPG format, raw or calibrated as available, following a brief pre-selection by OSIRIS scientists. Basic ‘metadata’ stating the date, time, distance to the comet and the Sun, and the resolution of the image will be included with each.

There will not be a detailed scientific description of the images because the goal is to provide up-to-date ‘postcards’ of the comet. Traditional image releases with scientific interpretation will still be made, separately, in the usual way.

The images will also be added to our ESA galleries and shared on our Rosetta social media channels. In addition, we plan to showcase them in a weekly blog post alongside our regular navigation camera (NavCam) CometWatch feature.

“This new initiative is a welcome addition to our long-established NavCam CometWatch releases, and gives us another way to enjoy riding along with Rosetta as it follows the comet through the Solar System,” notes Patrick Martin, ESA’s Rosetta mission manager.

“Now that we’re closer to the comet again we’re looking forward to seeing its surface in more detail. We’re also looking forward to sharing a fantastic view as Rosetta descends to the surface of the comet next September,” says Matt Taylor, ESA’s Rosetta project scientist.

Subscribe to the mailing list by emailing your request to: osiris-pi@mps.mpg.de

Visit the website at: https://planetgate.mps.mpg.de:8114/Image_of_the_Day/public/

Notes for Editors:

The OSIRIS dataset from both the wide- and narrow-angle cameras covering the period 20 June 2014 – 16 September 2014 are currently in processing and are foreseen for release via the Archive Image Browser and the Planetary Science Archive early next week.

For more information about Rosetta mission, visit: http://www.esa.int/Our_Activities/Space_Science/Rosetta

Rosetta overview: http://www.esa.int/Our_Activities/Space_Science/Rosetta_overview

Rosetta in depth:http://sci.esa.int/rosetta

Rosetta factsheet: http://www.esa.int/Our_Activities/Space_Science/Rosetta/Rosetta_factsheet

Frequently asked questions: http://www.esa.int/Our_Activities/Space_Science/Rosetta/Frequently_asked_questions

Image, Text, Credits: ESA/Rosetta/MPS for OSIRIS Team MPS/UPD/LAM/IAA/SSO/INTA/UPM/DASP/IDA.

Best regards, Orbiter.ch

Expedition 45 Crew Members Return Home












ROSCOSMOS - Soyuz TMA-17M Mission patch.

Dec. 11, 2015

The Crew before embarking aboard the Soyuz TMA-17M spacecraft. Image Credit: NASA

Expedition 45 Flight Engineer Kjell Lindgren of NASA is among three crew members who returned to Earth Friday after a 141-day mission aboard the International Space Station, landing in Kazakhstan at approximately 8:12 a.m. EST (7:12 p.m. Kazakhstan time).

Welcome Back to Earth

Also returning were Flight Engineers Oleg Kononenko of Roscosmos (Russian Federal Space Agency) and Kimiya Yui of the Japan Aerospace Exploration Agency (JAXA). The crew touched down northeast of the remote town of Dzhezkazgan in Kazakhstan, marking the first crew landing to occur after sunset and only the sixth nighttime Soyuz spacecraft return from the space station.

With the end of this mission, Kononenko now has spent 533 days in space, and Lindgren and Yui, both on their first flight, have spent 141 days in space.

While on station, the crew members participated in Earth observations and conducted research in the areas of physical, biological and molecular science to advance knowledge and demonstrate new technologies. Such investigations enable research breakthroughs and drive technology innovations that provide benefits on Earth, and will enable long-duration human and robotic exploration missions into deep space.


Image above: Expedition 45 crew members Kjell Lindgren of NASA, Oleg Kononenko of the Russian Federal Space Agency and Kimiya Yui of the Japan Aerospace Exploration Agency settle into the Soyuz TMA-17M spacecraft that carried them safely back to Earth on Dec. 11, 2015 after their 141-day mission aboard the International Space Station. Image Credit: NASA.

The space station is a test bed to demonstrate new technologies, and Lindgren and Yui took part in the Veggie plant growth experiment that yielded fresh lettuce for crew consumption in August. NASA is maturing Veggie technology aboard the space station to provide future pioneers with a sustainable food supplement -- a critical part of NASA’s journey to Mars.

As NASA moves toward long-duration exploration missions farther into the solar system, Veggie will be a resource for crew food growth and consumption. The system also could be used by astronauts for recreational gardening activities during deep space missions and may have implications for improving growth and biomass production on Earth, benefiting the average citizen.


Image above: Expedition 46 Commander Scott Kelly of NASA captured this image, from aboard the International Space Station, of the Dec. 11 undocking and departure of the Soyuz TMA-17M carrying home Expedition 45 crew members Kjell Lindgren of NASA, Oleg Kononenko of the Russian Federal Space Agency and Kimiya Yui of the Japan Aerospace Exploration Agency after their 141-day mission on the orbital laboratory. Image Credits: NASA/Scott Kelly.

Another key research area during Expedition 45 is the continued one-year mission with NASA astronaut Scott Kelly and Roscosmos’ Mikhail Kornienko that is providing insight into human health management for long-duration space travel

The crew members also welcomed three cargo spacecraft during their mission. The fifth Japanese HTV cargo craft brought several tons of supplies to the station in August, and in October, a Russian ISS Progress cargo craft docked to the station, also bringing tons of supplies. On Dec. 9, Lindgren led the grapple of Orbital ATK’s Cygnus spacecraft to the station, the U.S. company's fourth commercial resupply mission for NASA.


Image above: NASA astronaut Kjell Lindgren makes his first call home after landing in a Soyuz TMA-17M in Kazakhstan Dec. 11, 2015 after his 141-day mission aboard the International Space Station. Image Credit: NASA TV.

During his time on the orbiting complex, Lindgren ventured outside the confines of the space station for two planned spacewalks. The first included a variety of station upgrade and maintenance tasks, including routing cables to prepare for new docking ports for U.S. commercial crew spacecraft. The second spacewalk resulted in the successful reconfiguration of a space station ammonia cooling system.

Expedition 46 continues operating the station, with Kelly in command. Along with Kornienko and Sergey Volkov of Roscosmos, the three-person crew will operate the station for four days until the arrival of three new crew members. NASA astronaut Tim Kopra, Russian cosmonaut Yuri Malenchenko and Tim Peake of ESA (European Space Agency) are scheduled to launch from Baikonur, Kazakhstan, on Dec. 15.

Related article:

Veggie plant growth experiment: http://orbiterchspacenews.blogspot.ch/2015/08/meals-ready-to-eat-expedition-44-crew.html

Related links:

NASA’s journey to Mars: https://www.nasa.gov/content/nasas-journey-to-mars

One-year mission: https://www.nasa.gov/1ym/research

For more information about the space station, including media resources, visit: http://www.nasa.gov/station

For breaking news and features, follow the station on Twitter: https://twitter.com/Space_Station 

Images (mentioned), Video, Text, Credits: NASA/Stephanie Schierholz/NASA TV/Johnson Space Center/Dan Huot/Karen Northon.

Best regards, Orbiter.ch

NASA Mars Rover Curiosity Reaches Sand Dunes












NASA - Mars Science Laboratory (MSL) patch.

December 11, 2015

Fast Facts:

- Curiosity is using its wheels, as well as its science payload, to investigate sand that forms active dunes on Mars.

- Plans call for the rover to scoop up and sieve sand for onboard laboratory analysis.

NASA's Curiosity Mars rover has begun an up-close investigation of dark sand dunes up to two stories tall. The dunes are on the rover's trek up the lower portion of a layered Martian mountain.

A view of the rippled surface of what's been informally named "High Dune"

Image above: The rippled surface of the first Martian sand dune ever studied up close fills this Nov. 27, 2015, view of "High Dune" from the Mast Camera on NASA's Curiosity rover. Image Credit: NASA/JPL-Caltech/MSSS.

A wheel track exposing material beneath the surface of a sand sheet nearby

Image above: A wheel track left by NASA's Curiosity Mars rover exposes underlying material in a shallow sand sheet in this Dec. 2, 2015, view from Curiosity's Mast Camera (Mastcam). Image Credit: NASA/JPL-Caltech/MSSS.

The dunes close to Curiosity's current location are part of "Bagnold Dunes," a band along the northwestern flank of Mount Sharp inside Gale Crater. Observations of this dune field from orbit show that edges of individual dunes move as much as 3 feet (1 meter) per Earth year.


Image above: This view shows grains of sand where NASA's Curiosity Mars rover was driven into a shallow sand sheet near a large dune. Image Credit: NASA/JPL-Caltech/MSSS.

The rover's planned investigations include scooping a sample of the dune material for analysis with laboratory instruments inside Curiosity.


Image above: This Dec. 5, 2015, view of the undisturbed surface of a Martian sand dune called "High Dune" shows coarse grains remaining on the surface after wind removal of smaller particles. Image Credit: NASA/JPL-Caltech/MSSS.

Curiosity has been working on Mars since early August 2012. It reached the base of Mount Sharp in 2014 after fruitfully investigating outcrops closer to its landing site and then trekking to the mountain. The main mission objective now is to examine successively higher layers of Mount Sharp.

For more information about Curiosity, visit: http://mars.jpl.nasa.gov/msl

Images (mentioned), Text, Credits: NASA/Dwayne Brown/Laurie Cantillo/JPL/Guy Webster.

Greetings, Orbiter.ch

jeudi 10 décembre 2015

Pluto’s Close-up, Now in Color & Zooming in on Pluto’s Pattern of Pits












NASA - New Horizons Mission logo.

Dec. 10, 2015

Pluto’s Close-up, Now in Color. Image Credits: NASA/JHUAPL/SwRI

This enhanced color mosaic combines some of the sharpest views of Pluto that NASA’s New Horizons spacecraft obtained during its July 14 flyby. The pictures are part of a sequence taken near New Horizons’ closest approach to Pluto, with resolutions of about 250-280 feet (77-85 meters) per pixel – revealing features smaller than half a city block on Pluto’s surface. Lower resolution color data (at about 2,066 feet, or 630 meters, per pixel) were added to create this new image.

The images form a strip 50 miles (80 kilometers) wide, trending (top to bottom) from the edge of “badlands” northwest of the informally named Sputnik Planum, across the al-Idrisi mountains, onto the shoreline of Pluto’s “heart” feature, and just into its icy plains. They combine pictures from the telescopic Long Range Reconnaissance Imager (LORRI) taken approximately 15 minutes before New Horizons’ closest approach to Pluto, with  – from a range of only 10,000 miles (17,000 kilometers) – with color data (in near-infrared, red and blue) gathered by the Ralph/Multispectral Visible Imaging Camera (MVIC) 25 minutes before the LORRI pictures.

The wide variety of cratered, mountainous and glacial terrains seen here gives scientists and the public alike a breathtaking, super-high-resolution color window into Pluto’s geology.

Zooming in on Pluto’s Pattern of Pits. Image Credits: NASA/JHUAPL/SwRI

On July 14 the telescopic camera on NASA’s New Horizons spacecraft took the highest resolution images ever obtained of the intricate pattern of “pits” across a section of Pluto’s prominent heart-shaped region, informally named Tombaugh Regio. Mission scientists believe these mysterious indentations may form through a combination of ice fracturing and evaporation. The scarcity of overlying impact craters in this area also leads scientists to conclude that these pits – typically hundreds of yards across and tens of yards deep – formed relatively recently. Their alignment provides clues about the ice flow and the exchange of nitrogen and other volatile materials between the surface and the atmosphere.


Image above: On July 14 the telescopic camera on NASA’s New Horizons spacecraft took the highest resolution images ever obtained of the intricate pattern of “pits” across a section of Pluto’s prominent heart-shaped region, informally named Tombaugh Regio. The image is part of a sequence taken by New Horizons’ Long Range Reconnaissance Imager (LORRI) as the spacecraft passed within 9,550 miles (15,400 kilometers) of Pluto’s surface, just 13 minutes before the time of closest approach. Image Credits: NASA/JHUAPL/SwRI.

The image is part of a sequence taken by New Horizons’ Long Range Reconnaissance Imager (LORRI) as the spacecraft passed within 9,550 miles (15,400 kilometers) of Pluto’s surface, just 13 minutes before the time of closest approach. The small box on the global view shows the section of the region imaged in the southeast corner of the giant ice sheet informally named Sputnik Planum. The magnified view is 50-by-50 miles (80-by-80 kilometers) across. The large ring-like structure near the bottom right of the magnified view -- and the smaller one near the bottom left -- may be remnant craters. The upper-left quadrant of the image shows the border between the relatively smooth Sputnik Planum ice sheet and the pitted area, with a series of hills forming slightly inside this unusual “shoreline.”

For more information about New Horizons mission, visit: http://www.nasa.gov/mission_pages/newhorizons/main/index.html

Images (mentioned), Text, Credits: NASA/Bill Keeter.

Greetings, Orbiter.ch