jeudi 12 janvier 2017
Second Power Upgrade Spacewalk Starts Friday Morning
ISS - Expedition 50 Mission patch.
January 12, 2017
Expedition 50 astronauts Shane Kimbrough and Thomas Pesquet are ready for their mission’s second spacewalk that starts Friday at 7 a.m. EST. The duo will wrap up power maintenance work to connect new lithium-ion batteries and install adapter plates. Kimbrough and NASA astronaut Peggy Whitson started that work last Friday during a six-hour, 32-minute spacewalk. Live broadcasting at: https://www.nasa.gov/multimedia/nasatv/index.html
Both spacewalks complement the ongoing robotics work that started at the end of December. Ground controllers have been remotely-operating the Canadarm2 robotic arm and Dextre robotic hand to remove and stow the old nickel-hydrogen batteries and the install the new batteries.
Image above: Astronaut Thomas Pesquet (center) assists spacewalkers Peggy Whitson (left) and Shane Kimbrough in the U.S. Quest airlock on Jan. 6, 2017. Image Credit: NASA.
The three cosmonauts have been staying focused on their set of Russian space research and lab maintenance. Station veterans Andrey Borisenko and Oleg Novitskiy collected blood samples for a pair human research studies looking at bone loss and stress responses caused by living in space. First-time station resident Sergy Ryzhikov explored chemical reactions caused by jet engine exhaust in the Earth’s upper atmosphere.
Related article:
U.S. and French Astronauts Prep for Friday Spacewalk
http://orbiterchspacenews.blogspot.ch/2017/01/us-and-french-astronauts-prep-for.html
Related Links:
Bone loss: http://www.energia.ru/en/iss/researches/human/21.html
Stress responses: http://www.energia.ru/en/iss/researches/human/22.html
Chemical reactions: http://www.energia.ru/en/iss/researches/study/07.html
Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/index.html
International Space Station (ISS): https://www.nasa.gov/mission_pages/station/main/index.html
Image (mentioned), Text, Credits: NASA/Mark Garcia.
Greetings, Orbiter.ch
Huygens: 'Ground Truth' From an Alien Moon
NASA & ESA - Cassini-Huygens Mission to Saturn & Titan patch.
January 12, 2017
2005 Historic Descent to Titan Revisited
After a two-and-a-half-hour descent, the metallic, saucer-shaped spacecraft came to rest with a thud on a dark floodplain covered in cobbles of water ice, in temperatures hundreds of degrees below freezing. The alien probe worked frantically to collect and transmit images and data about its environs -- in mere minutes its mothership would drop below the local horizon, cutting off its link to the home world and silencing its voice forever.
Titan Touchdown
Although it may seem the stuff of science fiction, this scene played out 12 years ago on the surface of Saturn's largest moon, Titan. The "aliens" who built the probe were us. This was the triumphant landing of ESA's Huygens probe.
Huygens, a project of the European Space Agency, traveled to Titan as the companion to NASA's Cassini spacecraft, and then separated from its mothership on Dec. 24, 2004, for a 20-day coast toward its destiny at Titan.
The probe sampled Titan's dense, hazy atmosphere as it slowly rotated beneath its parachutes, analyzing the complex organic chemistry and measuring winds. It also took hundreds of images during the descent, revealing bright, rugged highlands that were crosscut by dark drainage channels and steep ravines. The area where the probe touched down was a dark, granular surface, which resembled a dry lakebed.
Thoughts on Huygens
Today the Huygens probe sits silently on the frigid surface of Titan, its mission concluded mere hours after touchdown, while the Cassini spacecraft continues the exploration of Titan from above as part of its mission to learn more about Saturn and its moons. Now in its dramatic final year, the spacecraft's own journey will conclude on September 15 with a fateful plunge into Saturn's atmosphere.
Image above: Images taken by Huygens were used to create this view, which shows the probe's perspective from an altitude of about 6 miles (10 kilometers). Image credits: ESA/NASA/JPL/University of Arizona.
With the mission heading into its home stretch, Cassini team members and NASA leaders look back fondly on the significance of Huygens:
"The Huygens descent and landing represented a major breakthrough in our exploration of Titan as well as the first soft landing on an outer-planet moon. It completely changed our understanding of this haze-covered ocean world." -- Linda Spilker, Cassini project scientist at NASA's Jet Propulsion Laboratory, Pasadena, California
"The Huygens images were everything our images from orbit were not. Instead of hazy, sinuous features that we could only guess were streams and drainage channels, here was incontrovertible evidence that at some point in Titan's history -- and perhaps even now -- there were flowing liquid hydrocarbons on the surface. Huygens' images became a Rosetta stone for helping us interpret our subsequent findings on Titan." -- Carolyn Porco, Cassini imaging team lead at Space Science Institute, Boulder, Colorado
"Cassini and Huygens have shown us that Titan is an amazing world with a landscape that mimics Earth in many ways. During its descent, the Huygens probe captured views that demonstrated an entirely new dimension to that comparison and highlights that there is so much more we have yet to discover. For me, Huygens has emphasized why it is so important that we continue to explore Titan." -- Alex Hayes, a Cassini scientist at Cornell University, Ithaca, New York
"Twelve years ago, a small probe touched down on an orangish, alien world in the outer solar system, marking humankind's most distant landing to date. Studying Titan helps us tease out the potential of habitability of this tiny world and better understand the chemistry of the early Earth." -- Jim Green, director of planetary science at NASA Headquarters, Washington
A collection of Huygens' top science findings is available from ESA at:
http://sci.esa.int/huygens-titan-science-highlights
The Cassini-Huygens mission is a cooperative project of NASA, ESA (European Space Agency) and the Italian Space Agency. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington. JPL designed, developed and assembled the Cassini orbiter.
More information about Cassini:
http://www.nasa.gov/cassini
http://saturn.jpl.nasa.gov
http://www.esa.int/Our_Activities/Space_Science/Cassini-Huygens
Image (mentioned), Video, Text, Credits: NASA/ESA/Markus Bauer/JPL/Preston Dyches.
Best regards, Orbiter.ch
mercredi 11 janvier 2017
U.S. and French Astronauts Prep for Friday Spacewalk
ISS - Expedition 50 Mission patch.
January 11, 2017
Commander Shane Kimbrough is getting ready for his second spacewalk in a week to complete the upgrade of power systems on the International Space Station. He will be joined by Thomas Pesquet from the European Space Agency who will be conducting his first spacewalk.
ESA astronaut Thomas Pesquet is set for his first spacewalk, on Friday 13 January. Together with NASA astronaut Shane Kimbrough, he will exit the International Space Station at 12:05 GMT (13:05 CET) to complete a battery upgrade to the outpost’s power system. Live broadcasting at: https://www.nasa.gov/multimedia/nasatv/index.html
The spacewalking duo are partnering up today with NASA astronaut Peggy Whitson to review Friday morning’s spacewalk. Whitson, who completed her seventh spacewalk last Friday, and cosmonaut Oleg Novitskiy will be assisting the spacewalkers in and out of their spacesuits and the Quest airlock.
Image above: Astronaut Shane Kimbrough is pictured during the first power upgrade spacewalk on Jan. 6, 2017. Image Credit: NASA.
Late yesterday and last night robotic ground controllers used the Dextre Special Purpose Dexterous Manipulator to move the final lithium-ion battery to the 1A power channel Integrated Electronics Assembly, moved another nickel-hydrogen battery to one of Dextre’s arms for temporary stowage and tightened down bolts on two of the previously moved Li-ion batteries.
So, we now have five nickel-hydrogen batteries either on the HTV External Pallet or temporarily stowed on Dextre and one more Ni-H battery to move from the 1A IEA to another stowage position on Dextre later today to complete the pre-EVA robotics. All six new lithium-ion batteries are now installed on the S4 truss IEA. The 3A power channel is fully operational. The 1A power channel will be activated on Friday during the EVA after adapter plates are moved into place on the 1A IEA.
Post-EVA robotics on Saturday and Sunday will complete the work to move the last four old Ni-H batteries from Dextre to the External Pallet for disposal (there will be nine on the EP in all). They will burn up in the Earth’s atmosphere when the HTV is deorbited.
Animated Earth views seen from ISS. Animation Credit: NASA
Whitson and Pesquet started their day scanning their arteries with and ultrasound and collecting body fluid samples for the Cardio Ox study. That experiment is researching the increased risk of atherosclerosis, the plaque build-up in the artery wall that results in narrowing of the blood vessel, in astronauts living in space.
In the Russian segment of the space station, cosmonaut Sergey Ryzhikov set up gear for a Matryoshka radiation detection experiment. Veteran cosmonaut Andrey Borisenko studied how mission events affect the station structure and explored new Earth photography techniques.
Related links:
Cardio Ox study: https://www.nasa.gov/mission_pages/station/research/experiments/931.html
Matryoshka radiation detection experiment: http://www.energia.ru/en/iss/researches/human/03.html
New Earth photography techniques: http://www.energia.ru/en/iss/researches/develop/04.html
Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/index.html
International Space Station (ISS): https://www.nasa.gov/mission_pages/station/main/index.html
Image (mentioned), Animation (mentioned), Text, Credits: NASA/Mark Garcia.
Best regards, Orbiter.ch
NASA Study Finds a Connection Between Wildfires and Drought
NASA - Suomi NPP Mission logo.
Jan. 11, 2017
For centuries drought has come and gone across northern sub-Saharan Africa. In recent years, water shortages have been most severe in the Sahel—a band of semi-arid land situated just south of the Sahara Desert and stretching coast-to-coast across the continent, from Senegal and Mauritania in the west to Sudan and Eritrea in the east. Drought struck the Sahel most recently in 2012, triggering food shortages for millions of people due to crop failure and soaring food prices.
Various factors influence these African droughts, both natural and human-caused. A periodic temperature shift in the Atlantic Ocean, known as the Atlantic Multi-decadal Oscillation, plays a role, as does overgrazing, which reduces vegetative cover, and therefore the ability of the soil to retain moisture. By replacing vegetative cover’s moist soil, which contributes water vapor to the atmosphere to help generate rainfall, with bare, shiny desert soil that merely reflects sunlight directly back into space, the capacity for rainfall is diminished.
Image above: Numerous fires create a smoky pall over the skies of western Africa. The image above was acquired on December 10, 2015. Image Credits: NASA Earth Observatory image by Joshua Stevens, using VIIRS data from Suomi NPP.
Another human-caused culprit is biomass burning, as herders burn land to stimulate grass growth, and farmers burn the landscape to convert terrain into farming land and to get rid of unwanted biomass after the harvest season. As with overgrazing, fires dry out the soil and stymie the convection that brings rainfall. Small particles called aerosols that are released into the air by smoke may also reduce the likelihood of rainfall. This can happen because water vapor in the atmosphere condenses on certain types and sizes of aerosols called cloud condensation nuclei to form clouds; when enough water vapor accumulates, rain droplets are formed. But have too many aerosols and the water vapor is spread out more diffusely to the point where rain droplets don’t materialize.
The relationship between fire and the water in northern sub-Saharan Africa, however, had never been comprehensively investigated until recently. A study published in the journal Environmental Research Letters, led by Charles Ichoku, a senior scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, seeks to shed light on the connection.
“We wanted to look at the general impacts of burning on the whole spectrum of the water cycle,” said Ichoku.
To do so, Ichoku and his colleagues used satellite records from 2001 to 2014 — including data from NASA’s Moderate Resolution Imaging Spectroradiometer and the Tropical Rainfall Measurement Mission — to analyze the impact of fires on various water cycle indicators, namely soil moisture, precipitation, evapotranspiration and vegetation greenness. Other work performed by the group focused more closely on examining the interactions between clouds and smoke and also the effects of fires on surface brightness.
Image above: The Suomi NPP satellite detected these fires (red dots) in Africa on January 30, 2016. Ichoku hypothesizes that such fires play a significant role in altering rainfall patterns. Image Credits: NASA Earth Observatory map by Joshua Stevens, using VIIRS data from Suomi NPP.
When Ichoku used satellite data to match fire activity to hydrological indicators, a pattern emerged. “There is a tendency for the net influence of fire to suppress precipitation in northern sub-Saharan Africa,” he said.
For example, in years that had more than average burning during the dry season, measurements of soil moisture, evaporation and vegetation greenness—all of which help to trigger rain—decreased in the following wet season. Even within dry seasons, the amount of water decreased in areas with more humid climates as the burning became more severe.
The results so far show only a correlation between fires and water cycle indicators, but the data gathered from the study is allowing scientists to improve climate models to be able to establish a more direct relationship between biomass burning and its impacts on drought.
For example, the research team is now incorporating the rate of radiant heat output from fires as well as the rate of fire-induced land-cover conversion into regional models, including the NASA Unified Weather Research and Forecasting model. Such new capability will enable the simulation of real fire impacts on drought.
Future modeling may explain some of the study’s seemingly paradoxical findings, including the fact that, even as fires decreased by 2 to 7 percent each year from 2006 to 2013, precipitation during those years did not increase proportionately.
Suomi NPP satellite. Image Credit: NASA
Ichoku thinks one possible reason a decrease in fires didn’t result in more precipitation has to do with the change in the types of lands that are being burned. The study found that throughout the same period, more forests and wetlands were being converted to cropland than in previous years. He notes that recent droughts have drawn people to farm areas that have more water. The drawback is that such land types provide a significant amount of moisture to the atmosphere that eventually becomes rain, so their conversion to farmland poses a threat to future water availability.
“The removal of vegetal cover through burning would likely increase water runoff when it rains, potentially reducing their water retention capacity and invariably the soil moisture,” Ichoku said. “The resulting farming would likely deplete rather than conserve the residual moisture, and in some cases, may even require irrigation. Therefore, such land cover conversions can potentially exacerbate the drought.”
To read the paper, visit:
http://iopscience.iop.org/article/10.1088/1748-9326/11/9/095005/meta
For more information about NASA Earth science research, visit: http://www.nasa.gov/earth
Suomi NPP satellite: https://jointmission.gsfc.nasa.gov/
Images (mentioned), Text, Credits: NASA’s Earth Science News Team, by Samson Reiny/Karl Hille.
Greetings, Orbiter.ch
mardi 10 janvier 2017
Weekly Recap From the Expedition Lead Scientist, Week of Dec. 26, 2016
ISS - Expedition 50 Mission patch.
Jan. 10, 2017
(Highlights: Week of Dec. 26, 2016) - The end of the calendar year also brought the end to another successful season of vegetable growth on the International Space Station.
NASA astronaut Shane Kimbrough completed the third and final harvest of red lettuce to close out the Veg-03 investigation. Understanding how plants respond to microgravity is an important step for future long-duration space missions, which will require crew members to grow their own food. Crew members on the station have previously grown lettuce and flowers in the Veggie facility. This new series of the study expands on previous validation tests. After collecting the lettuce, Kimbrough cleaned and powered down the Veggie facility.
Image above: NASA astronaut Shane Kimbrough collected the third and final harvest of this round of the Veggie investigation, testing the capability to grow fresh vegetables on the International Space Station. He is seen here, floating with some of the lettuce leaves aboard the station. Image Credit: NASA.
Veggie provides lighting and necessary nutrients for plants in the form of a low-cost growth chamber and planting pillows, which deliver nutrients to the root system. The Veggie pillow concept is a low-maintenance, modular system that requires no additional energy beyond a special light to help the plants grow. It supports a variety of plant species that can be cultivated for fresh food, and even for education experiments.
Crew members have commented that they enjoy space gardening, and investigators believe growing plants could provide a psychological benefit to crew members on long-duration missions, just as gardening is often an enjoyable hobby for people on Earth. Data from this investigation could benefit agricultural practices on Earth by designing systems that use valuable resources such as water more efficiently.
Image above: ESA astronaut Thomas Pesquet uses a long-lens camera to capture Earth observations from a window in the Russian Zvezda module. The Crew Earth Observation investigation is one of the longest-running investigations aboard the space station. Image Credit: NASA.
A ground team commanded the Additive Manufacturing Facility (Manufacturing Device) on the space station to print two items: a sample build for future materials studies and a design that was part of a student contest. Installed on the station in 2015, the Manufacturing Device is a 3-D printer that uses additive manufacturing to build a part layer by layer using an engineered plastic polymer as raw material.
The Manufacturing Device is another step toward a permanent manufacturing capability on the space station. It will enable the production of components and tools on demand in orbit, which will allow further research into manufacturing for long-term missions. The station crew can use it to print a variety of items to perform maintenance, build tools and repair sections in case of an emergency, leading to a reduction in cost, mass, labor and production time. Further research will also help develop this advanced technology for use on Earth.
Image above: NASA astronaut Shane Kimbrough works on the Combustion Integration Rack (CIR). CIR includes an optics bench, combustion chamber, fuel and oxidizer control, and five different cameras for performing combustion experiments in microgravity. Image Credit: NASA.
NASA astronaut Peggy Whitson retrieved the passive air samplers for the Aerosol Sampling experiment, stowing them for return to Earth. Aerosols are small particles suspended in the air. In Earth’s atmosphere, aerosols include soot, dust, pollen and a wide range of other natural and human-made materials. Smoke does not rise and dust does not settle in microgravity the way they do on Earth, causing aerosols to behave differently and posing hazards for crew members breathing the air. Aerosol Sampler collects airborne particles in the station’s air and returns them to Earth so scientists can study the particles with powerful microscopes. For this experiment, particles collected from cabin air are analyzed using a variety of microscopic techniques. Studying these particulates can allow scientists to improve the design of monitors for long-duration missions and help create better fire detectors that can discriminate between dust or background particles and smoke in order to reduce false alarms.
ISS - International Space Station. Animation Credit: NASA
Progress was made on other investigations and facilities this week, including Alpha Magnetic Spectrometer, Meteor, Education Payload Operations-Pesquet, ISS Ham, Packed Bed Reactor Experiment (PBRE), Skinsuit, Electrostatic Levitation Furnace (ELF), JAXA Small Satellite Orbital Deployer (J-SSOD), and Combustion Integrated Rack.
Crew members conducted other human research investigations this week, including Habitability, Fine Motor Skills, Fluid Shifts, Dose Tracker and Space Headaches.
Related links:
Veg-03 investigation: http://www.nasa.gov/mission_pages/station/research/experiments/1294.html
Additive Manufacturing Facility (Manufacturing Device): http://www.nasa.gov/mission_pages/station/research/experiments/2198.html
Aerosol Sampling experiment: https://www.nasa.gov/mission_pages/station/research/experiments/2300.html
Alpha Magnetic Spectrometer (AMS): https://www.nasa.gov/mission_pages/station/research/experiments/742.html
Meteor: https://www.nasa.gov/mission_pages/station/research/experiments/1323.html
ISS Ham: http://www.nasa.gov/mission_pages/station/research/experiments/346.html
Packed Bed Reactor Experiment (PBRE): https://www.nasa.gov/mission_pages/station/research/experiments/1111.html
Skinsuit: https://www.nasa.gov/mission_pages/station/research/experiments/2081.html
Electrostatic Levitation Furnace (ELF): http://iss.jaxa.jp/en/kiboexp/pm/elf/
JAXA Small Satellite Orbital Deployer (J-SSOD): http://www.nasa.gov/mission_pages/station/research/experiments/J-SSOD.html
Combustion Integrated Rack: https://spaceflightsystems.grc.nasa.gov/sopo/ihho/psrp/fcf/cir/
Habitability: https://www.nasa.gov/mission_pages/station/research/experiments/1772.html
Fine Motor Skills: https://www.nasa.gov/mission_pages/station/research/experiments/1767.html
Fluid Shifts: https://www.nasa.gov/mission_pages/station/research/experiments/1257.html
Dose Tracker: http://www.nasa.gov/mission_pages/station/research/experiments/1933.html
Space Headaches: http://www.nasa.gov/mission_pages/station/research/experiments/181.html
Space Station Research and Technology: https://www.nasa.gov/mission_pages/station/research/index.html
International Space Station (ISS): https://www.nasa.gov/mission_pages/station/main/index.html
Images (mentioned), Animation (mentioned), Text, Credits: NASA/Kristine Rainey/John Love, Acting Lead Increment Scientist Expeditions 49 & 50.
Best regards, Orbiter.ch
Hubble's Front Row Seat When Galaxies Collide
Jan. 10, 2017
This delicate smudge in deep space is far more turbulent than it first appears. Known as IRAS 14348-1447 — a name derived in part from that of its discoverer, the Infrared Astronomical Satellite (IRAS for short) — this celestial object is actually a combination of two gas-rich spiral galaxies. This doomed duo approached one another too closely in the past, gravity causing them to affect and tug at each other and slowly, destructively, merge into one. The image was taken by Hubble’s Advanced Camera for Surveys (ACS).
IRAS 14348-1447 is located over a billion light-years away from us. It is one of the most gas-rich examples known of an ultraluminous infrared galaxy, a class of cosmic objects that shine characteristically — and incredibly — brightly in the infrared part of the spectrum. Almost 95% of the energy emitted by IRAS 14348-1447 is in the far-infrared!
The huge amount of molecular gas within IRAS 14348-1447 fuels its emission, and undergoes a number of dynamical processes as it interacts and moves around; these very same mechanisms are responsible for IRAS 14348-1447’s own whirling and ethereal appearance, creating prominent tails and wisps extending away from the main body of the galaxy.
For images and more information about Hubble, visit:
http://hubblesite.org/
http://www.nasa.gov/hubble
http://www.spacetelescope.org/
Image Credits: ESA/Hubble & NASA/Text Credits: European Space Agency/NASA/Karl Hille.
Best regards, Orbiter.ch
Asteroid sleuths go back to the future
Asteroid Watch logo.
10 January 2017
Careful sleuthing through decade-old images has enabled ESA’s asteroid team to decide that a newly discovered space rock poses little threat of hitting Earth any time soon.
Spotting a previously unknown asteroid for the first time always raises the big question: is there a risk it will impact Earth?
Looking up
Yet, upon discovery, analysts often have very little to go on. The initial image from the observatory, survey team or individual backyard astronomer who spotted the rock typically gives only basic information – its location in the sky and its brightness – and sometimes these aren’t known terribly accurately.
The most crucial information needed to determine with any degree of confidence whether it is a ‘near-Earth object’ (NEO) – and that it will miss Earth (or not) – is the new object’s path. And determining that requires a series images acquired over a period of days or even months.
“We need multiple follow-on images to compute the trajectory and make a risk estimate, but even then the uncertainty can be very large. It really takes many months of observations to get a good, reliable impact risk estimate, and in the meantime, there can be reason to worry,” says Ettore Perozzi of the NEO Coordination Centre at ESA’s facility in Italy.
Spotted from Arizona
This is precisely what happened on 19 October, when asteroid 2016 WJ1 was discovered by the Catalina Sky Survey.
Asteroid 2016 WJ1
“The additional images allowed us to refine our knowledge of the trajectory sufficiently to begin searching astronomical archives, to see if anyone had previously imaged this asteroid without having recognised it as such,” says Marco Micheli, observer at the NEO centre.
If any were found, the team would score what astronomers call a ‘precovery’ – short for pre-discovery.
Precovering
The investigation quickly bore fruit: images found online from the Pan-STARRS survey taken earlier in October showed what might be the target asteroid.
While these were inconclusive, the team assumed they were, in fact, accurate and then used these to call up additional, highly accurate images from a Canadian astronomical image search system.
Bingo: two sets of images from 4 and 5 July 2003 with the Canada–France–Hawaii Telescope were found.
ESA observatory
“After careful inspection we were able to pinpoint the object, and the team were able to perform some very accurate determinations,” says Detlef Koschny, responsible for the NEO portion of ESA’s Space Situational Awareness programme.
“The result was that we could preclude any risk of Earth impact from asteroid 2016 WJ1 anytime soon or well into the future.”
ESA is now developing a new set of automated, wide-field-of-view ‘Fly-Eye’ telescopes that will conduct nightly sky surveys, creating a large future archive of images that will make critical precovery confirmations more efficient in future.
Related links:
Catalina Sky Survey: http://www.lpl.arizona.edu/css/
Canada–France–Hawaii Telescope: http://www.cfht.hawaii.edu/
‘Fly-Eye’ telescopes: http://www.esa.int/ESA_Multimedia/Images/2016/10/Fly-eye_telescope
NASA NEO Office: http://neo.jpl.nasa.gov/
UNOOSA/UN-SPIDER: http://www.un-spider.org/
Minor Planet Center: http://www.minorplanetcenter.org/iau/mpc.html
Spaceguard Central Node: http://spaceguard.rm.iasf.cnr.it/
European Asteroid Research Node: http://earn.dlr.de/
Near-Earth Objects - Dynamic Site: http://newton.dm.unipi.it/neodys/
UK Spaceguard Centre: http://www.spaceguarduk.com/
Images, Text, Credits: ESA/Catalina Sky Survey, University of Arizona/Canada-France-Hawaii Telescope/StarryEarth via Flickr.
Greetings, Orbiter.ch
Inscription à :
Articles (Atom)