Copernical Team
Prepping for a spacewalk to install Colka on ISS external hull
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Prepping for a spacewalk typically means diving underwater to rehearse and fine-tune operations.
In 2016, ESA astronaut Alexander Gerst performed such an underwater rehearsal for the Colka high speed radio, the brown box imaged above, that will be installed this month on the International Space Station.
NASA astronauts Mike Hopkins and Victor Glover will integrate the small fridge-si Exotrail aims for more in orbit space mobility
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Exotrail reports full success of first-ever cubesat mission equipped with Hall-effect electric propulsion technology. Through an In-Orbit Demonstration mission launched to Low Earth Orbit on 7th of November 2020 onboard a PSLV rocket, Exotrail nominally ignited its ExoMGTM Hall-effect electric propulsion system on the first attempt.
Small satellite constellations will now be able to quickl Cheers! French wine, vines headed home after year in space
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The International Space Station bid adieu Tuesday to 12 bottles of French Bordeaux wine and hundreds of snippets of grapevines that spent a year orbiting the world in the name of science.
Curiosity rover reaches its 3,000th day on Mars
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As the rover has continued to ascend Mount Sharp, it's found distinctive benchlike rock formations.
It's been 3,000 Martian days, or sols, since Curiosity touched down on Mars on Aug. 6, 2012, and the rover keeps making new discoveries during its gradual climb up Mount Sharp, the 3-mile-tall (5-kilometer-tall) mountain it has been exploring since 2014. Geologists were intrigued to see a series of rock "benches" in the most recent panorama from the mission.
Stitched together from 122 images taken on Nov. 18, 2020, the mission's 2,946th sol, the panorama was captured by the Mast Camera, or Mastcam, which serves as the rover's main "eyes.
New Horizons spacecraft answers the question: How dark is space?
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Reconstructing the solar system's original architecture
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As the solar system was developing, the giant planets (Jupiter and Saturn) formed very early, and as they grew, they migrated both closer to and further away from the sun to stay in gravitationally stable orbits.
The gravitational effect of these massive objects caused immense reshuffling of other planetary bodies that were forming at the time, meaning that the current locations of many planetary bodies in our solar system are not where they originally formed.
Lawrence Livermore National Laboratory (LLNL) scientists set out to reconstruct these original formation locations by studying the isotopic compositions of different groups of meteorites that all derived from the asteroid belt (between Mars and Jupiter). The asteroid belt is the source of almost all of Earth's meteorites, but the material that makes up the asteroid belt formed from sweeping of materials all over the solar system.
SpaceX's next idea: Catch Super Heavy boosters with the launch tower
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SpaceX is getting closer and closer to realizing the design for its Starship and Super Heavy launch system. Once complete, it will be the world's first fully reusable launch system and will facilitate trips to low Earth orbit (LEO), the moon and Mars. Construction began on the system's booster element (Super Heavy) this past summer and, according to a recent tweet by Musk, will be "caught" by its launch tower.
The tweet came (as they often do) in response to a question from one of Musk's followers. In this case, it was a space designer who goes by the Twitter handle Erc X (@ErcXspace) who produced a video that illustrates what the Super Heavy might look like as it returns to its landing site. The video is captioned with a question: "Accurate Super Heavy Descent profile?"
Accurate Super Heavy Descent profile? pic.twitter.com/MxIJ0zLzKn
— Erc X (@ErcXspace) December 30, 2020
Musk responded by tweeting:
"We're going to try to catch the Super Heavy Booster with the launch tower arm, using the grid fins to take the load… Saves mass & cost of legs & enables immediate repositioning of booster on to launch mount—ready to refly in under an hour.
The obliquity of Mars: Periodic bedding in Tithonium Chasma
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Earth's seasons are caused by the tilt of our planet's rotational axis to the orbital plane or obliquity. Mars' obliquity is currently about 25 degrees, which is not much different from Earth's 23 degrees. However, numerical calculations by scientists at the Paris Observatory and Massachusetts Institute of Technology suggest that this near-agreement is a coincidence.
Under the influence of gravitational torques from other planets, Mars' obliquity varies chaotically, probably reaching values greater than 60 degrees and lower than 10 degrees. By contrast, Earth's obliquity appears to have been limited to small variations from its current value because of the stabilizing gravitational influence of the Moon. If the calculations are correct, then for most of the Solar System's history, the obliquity of Mars was greater than 25 degrees. This would produce warmer summers and colder winters than on present-day Mars. On Earth, a recent 1 degree rise in obliquity is believed to have triggered ice sheet retreat from the current location of New York City to Greenland. The climatic consequences of 50 degree changes in obliquity on Mars remain unknown.
It is possible, though unproven, that higher obliquity triggered partial melting of some of Mars' water ice.
Image: Frosty scenes in Martian summer
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The CaSSIS camera onboard the ExoMars Trace Gas Orbiter captured remnant frost deposits in a region near Sisyphi Tholus, in the high southern latitudes of Mars (74ºS/246ºE).
This image was taken during the early morning of a midsummer day in the southern hemisphere. At these high latitudes, carbon dioxide ice and frost develop. Frost can be seen within polygonal cracks in the terrain, a feature that indicates the presence of water ice embedded in the soil. The black spots observed throughout the scene are due to dark soil being pushed through cracks in the carbon dioxide ice as it sublimates—turns directly from solid ice to vapor—in the summer months.
The scale is indicated on the image.
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Energy from solar wind favors the north
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Using information from ESA's Swarm satellite constellation, scientists have made a discovery about how energy generated by electrically-charged particles in the solar wind flows into Earth's atmosphere—surprisingly, more of it heads towards the magnetic north pole than towards the magnetic south pole.
The sun bathes our planet with the light and heat to sustain life, but it also bombards us with dangerous charged particles in the solar wind.