When Artemis 1 finally takes flight (possibly this Saturday), twelve bags of baker’s yeast will go along for the ride. Millions of these cells of Saccharomyces cerevisiae will experience deep space as it grows and reproduces. The yeast is a stand-in for actual people. The idea is to see what threat the radiation environment in deep space poses to living cells. The data from the experiment will point to how genetic engineering might help reduce damage to astronauts.
The James Webb Space Telescope has taken its first direct image of an exoplanet, a planet outside our Solar System. The exoplanet, HIP 65425 b is a gas giant that orbits an A-type star, has a mass of about nine times that of Jupiter and is about 355 light-years from Earth. While the planet has virtually no chance of being habitable, the data from these observations show just how powerful a tool JWST will be for studying exoplanets.
A recent blog by Dr. Justin Maki, Imaging Scientist and the Deputy Principal Investigator on the Perseverance rover Mastcam-Z camera, provides a detailed account about the debris the entry, descent, and landing (EDL) system left scattered around the Martian surface while delivering the Perseverance rover to Jezero Crater. This blog highlights how much hardware goes into sending our brave, robotic explorers to the Red Planet while discussing the importance of imaging such debris.
A super-Earth planet has been found orbiting a red dwarf star, only 37 light-years from the Earth. Named Ross 508 b, the newly found world has an unusual elliptical orbit that causes it to shift in and out of the habitable zone. Therefore, part of the time conditions would be conducive for liquid water to exist on the planet’s surface, but other times it wouldn’t.
* Warning: Mild Spoilers Ahead *
Planetary nebulae are short-lived “leftovers” of sun-like stars. Most of these “star ghosts” only last—at most—about 25,000 years. Usually, their clouds of debris disperse so broadly that they fade out fairly quickly. However, there’s one that has lasted at least 70,000 years. That makes it a “grande dame” of planetary nebulae.
On February 18th, 2021, the Perseverance rover landed in the Jezero Crater on Mars. Since then, Perseverance has been exploring the region in search for evidence of past (and possibly present) life – much like its cousin, the Curiosity rover. This includes obtaining samples that will be placed in a cache and retrieved by a future ESA/NASA sample-return mission. These will be the first directly-retrieved samples of Martian rock and soil that will be analyzed in a laboratory on Earth, which are expected to reveal some tantalizing bits about the history of the Red Planet.
No, James Webb didn’t disprove the Big Bang. Carbon dioxide found in an exoplanet atmosphere. An amazing picture of Jupiter from Webb, pieces of other stars found in asteroid Ryugu, weak astronauts arriving on Mars, and a new way to measure distances in the Universe.
What’s the recipe for forming stars? Yep, lots of gas and dust. Galaxies rich in these materials get to make a lot of stars. When the supply runs out, star formation stops. That’s what’s happened in the galaxy SDSS J1448+1010, but there’s a twist. The galaxy didn’t stop making stars because it made so many it ran out of material. No, that happened because it merged with another galaxy. That action flung most of the available gas and dust out of the galaxy entirely. Essentially, the galaxy to went “dormant” and ceased star-forming operations.
Earlier this year, the teams attached to the Voyager 1 mission noticed that the venerable spacecraft was sending weird readouts about its attitude articulation and control system (called AACS, for short). The data it’s providing didn’t really reflect what was actually happening onboard. That was the bad news. The good news was that it didn’t affect science data-gathering and transmission. And, the best news came this week: team engineers have fixed the issue with the AACS and the data are flowing normally again.
As Artemis 1 prepares for its maiden launch with the goal of putting astronauts back on the Moon’s surface within the next few years, the next question is how will astronauts live and survive its surface? Will we constantly ferry all the necessary supplies such as water and food from Earth, or could astronauts learn to survive on their own? These are questions that a discipline known as ISRU hopes to answer both now and in the years to come. But what is ISRU, and how will it help advance human space exploration as we begin to slowly venture farther away from the only home we’ve ever known?
After reviewing the data from Monday’s scrubbed launch attempt for the Space Launch System/Artemis- 1 test flight, NASA’s Mission Management Team feels the rocket and the launch team will be ready for another try at the program’s maiden launch on Saturday, September 3. The two-hour launch window starts at 2:17 pm EDT (18:17 UTC).
What do MINBAR, TARDIS, Cardassian Expansion, BoRG, DS9, Tatooines, and ACBAR all have in common? They’re names of astronomical surveys and software created by astronomers who say that science fiction (SF) influenced their careers. Those names are just one indicator of widespread interest in SF in the science community. It’s not surprising considering how many scientists (and science writers) grew up with the genre.
The Perseverance rover is enjoying a bit of a winning streak lately! For the past year and a half, the rover has been exploring the Jezero crater on Mars to learn more about the planet’s past. As part of this mission, Perseverance is obtaining samples of Martian rock and soil that it will set aside in a cache for future retrieval. As part of a NASA/ESA sample-return mission, these will be returned to Earth for analysis and could contain evidence of past life. Thanks to the international team of geologists and astrobiologists overseeing the collection process, the first of these rock samples have been obtained!
SpaceX’s Starlink satellite system has been in the news lately for both good and ill. The “Mega-constellation” of around 2,800 satellites added another 53 satellites to its roster just last week. But while it might one day provide high-speed internet for the whole of humanity, it is already causing a massive headache for one particular slice of humanity – astronomers. Starlink satellites are reflective due to the solar panels they need to power themselves.
In a recent study published in Instrumentation and Methods for Astrophysics, the private space company, Rocket Lab, outlines a plan to send their high-energy Photon spacecraft to Venus in May 2023 with the primary goal of searching for life within the Venusian atmosphere. The planet Venus has become a recent hot topic in the field of astrobiology, which makes the high-energy Photon mission that much more exciting.
Addendum: Today’s launch was scrubbed due to an engine issue that occurred during fueling. The backup date of Sept. 2nd is now targeted.
In the search for extrasolar planets, astronomers and astrobiologists generally pursue a policy of “follow the water.” This comes down to searching for planets that orbit with a star’s circumsolar habitable zone (HZ), where conditions are warm enough that liquid water can flow on its surface. The reason is simple: water is the only known solvent capable of supporting life and is required by all life on Earth. However, since the 1970s, scientists have speculated that there may be a class of rocky planets in our Universe that are completely covered in water.
Because of the orbiters and landers that have studied Mars over the years, scientists have learned that water ice is very likely locked away just under the surface throughout the planet’s mid-latitudes. These regions – especially in the northern hemisphere — are mostly covered with smooth material and scientists suspect ice is just underneath.
In just four days, the inaugural mission of the Artemis Program will lift off from Kennedy Space Center in Florida! Dubbed Artemis I, this mission will see the Space Launch System (SLS) and Orion spacecraft achieve flight together for the first time. The mission will last between 39 and 42 days and consist of the uncrewed Orion flying beyond the Moon, farther than any spaceship has ever traveled, and then looping back around the Moon to return home. This flight, and the crewed Artemis II that will follow, are essentially the dress rehearsal for the long-awaited return to the Moon.
Protoplanetary disks—those nurseries around young stars where planets form—are filled with gas and dust. In particular, many show a lot of carbon monoxide gas. It’s a handy “tracer” to estimate the mass of a cloud, its composition, and even its temperature. It’s also easy to observe. However, astronomers think there should be more of it than they’re observing in many disks. And that prompted a question: where’s the rest of it?
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