Juno Just Saw a Spacerock Crash Into Jupiter

Timing is extraordinarily important in many aspects of astronomy.  If an astronomer or their instrument is looking the wrong way at the wrong time they could miss something spectacular.  Alternatively, there are moments when our instruments capture something unexpected in regions of space that we were searching for something else.  That is exactly what happened recently when a team of scientists, led by Rohini Giles at the Southwest Research Institute, saw an image of what is likely a meteor impacting Jupiter’s atmosphere.  

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The Largest Crater on the Moon Reveals Secrets About its Early History

Thorium concentrations measured by Lunar Prospector across the vast South Pole–Aitken Basin on the lunar far side are shown here, illustrating how mantle material ejected by an impact event about 4.3 billion years ago is currently distributed across the surface. Warmer colors represent higher concentrations; contour lines are at intervals of 0.5 part per million. Credit: Daniel P. Moriarty III

One of the oldest, deepest, and largest impact craters on the Moon provides a window into the history and makeup of our celestial companion, and needs to be studied in more detail, says a team of lunar scientists. The South Pole-Aitken Basin on the Moon formed from a gigantic impact about 4.3 billion years ago. Scientists say a more detailed analysis of this area will help refine the timeline of events in the Moon’s development, as well as help explain the dramatic differences between the lunar nearside and farside.

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NASA’s Perseverance Rover: The Most Ambitious Space Mission Ever?

Artist's impression of the Perseverance rover on Mars. Credit: NASA-JPL

When it comes to Mars exploration, NASA has more success than any other agency. This week, they’ll attempt to land another sophisticated rover on the Martian surface to continue the search for evidence of ancient life. The Mars Perseverance rover will land on Mars on Thursday, February 18th, and it’s bringing some very ambitious technologies with it.

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NASA’s InSight Will Have Reduced Capability Until a Dust Devil Cleans off its Solar Panels

Credit: NASA/JPL-Caltech

All eyes are on Mars this week, and, if we’re being honest, NASA’s InSight lander isn’t the star of the show right now. At the time of writing, we’re anxiously waiting to find out whether or not the Perseverance rover survives its fiery arrival at Mars. But Entry, Descent, and Landing (EDL) is just the first hazard that awaits robotic missions to the red planet. Mars exploration is a marathon, not a sprint, and while Perseverance is just getting started, InSight, which has been on the red planet for two years now, is approaching a tough leg of the race.

InSight’s nemesis: Martian dust. The same cruel villain that killed the Opportunity rover back in 2018.

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Water Shaped Features on Mars Much Earlier Than Previously Believed

Credit: NASA/JPL-Caltech

In two days (on Thursday, Feb. 18th, 2021), NASA’s Perseverance rover will land on Mars. As the latest robotic mission in the Mars Exploration Program (MEP), Perseverance will follow in the footsteps of its sister mission, Curiosity. Just in time for its arrival, research conducted at the Southwest Research Institute (SwRI) has shown that Mars’ surface was shaped by flowing water several million years earlier than previously thought.

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This is What Happens to Spacecraft When They Re-Enter the Earth’s Atmosphere

The Russian Progress 76P MS-15 cargo spacecraft, after undocking from the International Space Station and burned up in the atmosphere, asl planned in February 2021. Image via astronaut Soichi Noguchi.

When one of the Russian Progress resupply ships undocks from the International Space Station, timing is everything. The Progress needs to fire its engines at just the right time to instigate the deorbit burn in order for the ship to enter the atmosphere at just the right place, so that its destructive re-entry occurs over the Pacific Ocean. That way, any potential surviving bits and pieces that might reach Earth will hit far away from any land masses – which are home to people, buildings, and other things we don’t want to get bonked.

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The Surprising Discovery of Ceramic Chips Inside Meteorites Means There Were Wild Temperature Variations In the Early Solar System

A protosolar disk is the disk of material around a young stellar object that isn't yet a star. It's called a protoplanetary disk once the star has formed and begun fusion. Planetesimals are the building blocks of planets and are present in both stages of a disk's evolution. Image Credit: NASA/JPL

Meteorites are excellent windows into early solar system formation.  Many were formed in the those early days, and unlike rocks on the Earth, most are not affected by billions of years of tectonic activity that wipes away any of their original structure.  Recently a team led by Nicolas Dauphas and Justin Hu at the University of Chicago (UC) found that the formation process for many of these meteorites was much more violent than previously thought.

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A Combined Map of Almost 15,000 Dust Storms on Mars

Data in the world of astronomy is spread out in so many different places.  There are archives for instruments on individual spacecraft and telescopes.  Sometimes all that is needed to get new insight out of old data is to collect it all together and analyze a whole set rather than isolated instances.  That is exactly what happened recently when a team from the Harvard Center for Astrophysics collected and analyzed data about almost 15,000 dust storms that have taken place on Mars over the last eight Martian years.

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A Cluster of Black Holes Found Inside a Globular Cluster of Stars

This image from the NASA/ESA Hubble Space Telescope shows the central region of the rich globular star cluster NGC 3201 in the southern constellation of Vela (The Sails). A star that has been found to be orbiting a black hole with four times the mass of the Sun is indicated with blue circle. Credit: ESA/NASA

Black holes come in at least two sizes: small and large. Small black holes are formed from stars. When a large star reaches the end of its life, it typically ends in a supernova. The remnant core then collapses under its own weight, forming a black hole or neutron star. Small stellar-mass black holes are typically tens of solar masses. Large black holes lurk in the centers of galaxies. These supermassive black holes can be millions or billions of solar masses. They formed during the early universe and triggered the formation and evolution of galaxies around them.

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NASA has Decided to Start Building the Lunar Gateway Using the Falcon Heavy

An illustration of the Gateway’s Power and Propulsion Element and Habitation and Logistics Outpost in orbit around the Moon. Credits: NASA

In October of 2024, NASA will send “the first woman and the next man” to the Moon as part of the Artemis Program. This will be the first crewed mission to the lunar surface, and the first mission beyond Low Earth Orbit (LEO), since the closing of the Apollo Era in 1972. Beyond that, NASA plans to establish infrastructure on and around the Moon that will allow for “sustained lunar exploration and development.”

A key aspect of this is the Lunar Gateway, an orbiting habitat that will allow astronauts to make regular trips to and from the lunar surface. After much consideration, NASA recently announced that they have selected SpaceX to launch the foundational elements of the Gateway – the Power and Propulsion Element (PPE) and the Habitation and Logistics Outpost (HALO) – by May of 2024 (at the earliest).

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