Astronomers Create the First 3D Model of a Planet Orbiting in a Binary System

Artist's conception of an exoplanet about twice the size of Jupiter, the star it orbits, and the binary companion in the distance. Credit: Sophia Dagnello, NRAO/AUI/NSF.

To date, 5,084 extrasolar planets have been confirmed in 3,811 planetary systems, with another 8,912 candidates awaiting confirmation. These discoveries have provided astronomers with a detailed sampling of the types of planets that exist in our Universe, ranging from gas giants several times the size of Jupiter to smaller, rocky bodies like Earth. So far, the vast majority of these have been discovered using indirect methods – like the Transit Method (Transit Photometry) and the Radial Velocity Method (Doppler Spectroscopy) – while the remainder has been detected using various other means.

In a recent study, an international team of astronomers used the National Science Foundation’s (NSF) Very Long Baseline Array (VLBA) network to detect a Jupiter-like planet orbiting in a binary system (GJ 896AB) located about 20 light-years from Earth. Using a method known as Astrometry, the team managed to detect this planet by the “wobble” it makes as it orbits the larger of the system’s two stars. Moreover, this method allowed the team to create the first 3-dimensional architecture of a binary system and a planet that orbits one of its stars.

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Bouncy Castles on the Moon. Inflated Habitats Might be the Best Way to Get Started on a Lunar Base

In this decade, multiple space agencies will send astronauts to the Moon for the first time since the Apollo Era. In addition to NASA, the ESA, China, and Roscosmos, commercial space entities like SpaceX and Blue Origin are hoping to conduct regular missions in support of human exploration while also mounting their own private ventures. In time, this activity could result in the creation of permanent infrastructure, a regular human presence, and the emergence of a lunar economy. Nevertheless, there are many questions about how humans will live in lunar conditions and what type of facilities will be needed.

To this end, the Austrian-based inflatable structures specialist Pneumocell recently conducted a study to determine if lightweight prefabricated structures would be a suitable option. According to this study, a series of donut-shaped inflatable structures could be transported to the Moon at a low cost, where they would then be inflated. The habitats would be partially buried beneath the lunar regolith and surrounded by solar mirrors that could direct sunlight into their greenhouses. This “Inflatable Moon Habitat” offers a cost-effective and highly self-sufficient means of establishing a foothold on the Moon.

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Star Formation in the Center of the Milky Way Started at the Core and Then Worked its way out

False-color image of the region Sagittarius B1, as seen by the GALACTICNUCLEUS survey. Credit & ©: F. Nogueras-Lara et al. / MPIA

One of the biggest questions facing astronomers today concerns star formation and its role in the evolution of galaxies. In particular, astronomers are curious whether the process began in the central regions of galaxies, where stars are more tightly bound. Previous observations have shown that numerous galaxies experienced intense periods of star formation in their centers roughly one billion years after the Big Bang. For some time, astronomers have wanted to conduct similar observations of the Milky Way’s Galactic Center to study rapid star formation more closely.

Unfortunately, it has been very difficult for astronomers to study the center of the Milky Way because of how bright and densely packed the region is, which makes it difficult to discern individual stars and clusters. Thanks to a new analysis of a high-resolution infrared survey, a team of astronomers has created the first reconstruction of the star formation history in the Galactic Center. According to their findings, most young stars in this region formed in loose stellar associations that dispersed outwards to fill the Galactic Disk over the course of many eons (as opposed to tightly-knit massive clusters).

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Pulsars are Blasting out Cosmic Rays With a Million Billion Electronvolts

Distant past supernovae could be linked by cosmic ray particles to climate change on Earth and changes in biodiversity. Courtesy: Henrik Svensmark, DTU Space.
Distant past supernovae could be linked by cosmic ray particles to climate change on Earth and changes in biodiversity. Courtesy: Henrik Svensmark, DTU Space.

We are living in an exciting time, where next-generation instruments and improved methods are leading to discoveries in astronomy, astrophysics, planetary science, and cosmology. As we look farther and in greater detail into the cosmos, some of the most enduring mysteries are finally being answered. Of particular interest are cosmic rays, the tiny particles consisting of protons, atomic nuclei, or stray electrons that have been accelerated to near the speed of light. These particles represent a major hazard for astronauts venturing beyond Earth’s protective magnetic field.

At the same time, cosmic rays regularly interact with our atmosphere (producing “showers” of secondary particles) and may have even played a role in the evolution of life on Earth. Due to the way they carry an electric charge, which scrambles their path as they travel through the Milky Way’s magnetic field, astronomers have been hard-pressed to find where cosmic rays originate. But thanks to a new study that examined 12 years of data from NASA’s Fermi Gamma-ray Space Telescope, scientists have confirmed that the most powerful originate from shock waves caused by supernova remnants.

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The Geology at Jezero Crater is Even More Complex Than Scientists Were Expecting

After 5 years and 60 candidates, NASA has chosen Jezero crater as the landing site for the Mars 2020 rover. Image Credit: NASA/JPL/JHUAPL/MSSS/Brown University
After 5 years and 60 candidates, NASA has chosen Jezero crater as the landing site for the Mars 2020 rover. Image Credit: NASA/JPL/JHUAPL/MSSS/Brown University

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.

But it appears that we don’t need to wait on the sample-return mission since the Perseverance rover is already sending some surprising data back to Earth. According to a new study by a research team led by the University of California at Los Angeles (UCLA) and the University of Oslo, Perseverance’s ground-penetrating radar detected that the rock layers beneath the crater are strangely inclined. These strange sections could have resulted from lava flows that slowly cooled or could be sedimentary deposits from an underground lake.

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New Perseverance Rock Samples Were Altered by Water. They'll be Coming Back to Earth in the Sample Return Mission

Panoramic "selfie" view of the Perseverance rover and Ingenuity helicopter in the Jezero Crater, Mars. Credit: NASA/JPL-Caltech

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!

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Everything Still Looks Good for Monday's Artemis 1 Launch

NASA’s Space Launch System and Orion spacecraft for Artemis I on the pad at Launch Complex 39B at NASA’s Kennedy Space Center. Credit: NASA/Ben Smegelsky

Addendum: Today’s launch was scrubbed due to an engine issue that occurred during fueling. The backup date of Sept. 2nd is now targeted.

On Monday, August 29th, NASA will make history with the launch of the Artemis I mission. As the first flight in the Artemis Program, the mission will consist of a fully-stacked Space Launch System (SLS) and an Orion spacecraft taking off from Kennedy Space Center in Florida. Once in orbit, the uncrewed Orion spacecraft and European Space Module (ESM) will fly beyond the Moon before returning to Earth. This mission will validate the key systems and components of the Artemis Program and be a dress rehearsal for the crewed Artemis II mission in 2024.

According to the Flight Readiness Review, the Artemis I mission is a GO for launch and will launch no earlier than 02:33 PM EST (11:33 PM PST). While the mission is uncrewed, the crew module will still carry two mannequins (Helga and Zohar), occupying two of the capsule’s passenger seats. Helga and Zohar will carry over 5600 sensors to measure the radiation load during the circumlunar journey. Shaun the Sheep, a character from the popular animated series Wallace and Grommit, will occupy the third seat as part of a global social media campaign.

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Mechazilla Lifts a Super Heavy With all 33 Engines Onto the Launchpad

Mechazilla transports the fully-stacked Starship onto its launch pad. Credit: SpaceX

Little by little, SpaceX is getting closer to conducting the maiden orbital flight with its Starship and Super Heavy prototype! That was certainly the message Elon Musk conveyed on August 23rd when he posted an image via Twitter of the “Mechazilla” launch tower loading the fully-stacked prototype onto its launchpad at the SpaceX Starbase in Boca Chica, Texas. From here, the six-engine SN24 Starship and the BN7 Super Heavy prototype (with its full complement of 33 Raptor engines) will launch, which could happen in just a few weeks.

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A New Study Confirms That Gravity has Remained Constant for the Entire age of the Universe

The first image taken by the James Webb Space Telescope, featuring the galaxy cluster SMACS 0723. Credit: NASA, ESA, CSA, and STScI

For over a century, astronomers have known that the Universe has been expanding since the Big Bang. For the first eight billion years, the expansion rate was relatively consistent since it was held back by the force of gravitation. However, thanks to missions like the Hubble Space Telescope, astronomers have since learned that roughly five billion years ago, the rate of expansion has been accelerating. This led to the widely-accepted theory that a mysterious force is behind the expansion (known as Dark Energy), while some insist that the force of gravity may have changed over time.

This is a contentious hypothesis since it means that Einstein’s General Theory of Relativity (which has been validated nine ways from Sunday) is wrong. But according to a new study by the international Dark Energy Survey (DES) Collaboration, the nature of gravity has remained the same throughout the entire history of the Universe. These findings come shortly before two next-generation space telescopes (Nancy Grace Roman and Euclid) are sent to space to conduct even more precise measurements of gravity and its role in cosmic evolution.

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Astronomers Find a Waterworld Planet With Deep Oceans in the Habitable Zone

Artist's rendering of a super-Earth-type exoplanet, TOI 1452 b. Credit: Benoit Gougeon, Université de Montréal.

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.

With the explosion in confirmed exoplanets, scientists have been eager to find examples of this type of planet, so they study them more closely. Thanks to an international team of researchers led by the Institute for Research on Exoplanets (iREx) at the Université de Montréal, an exoplanet orbiting within its system’s HZ was recently discovered that could be completely covered in deep oceans. This “ocean world” (aka. “Waterworld”) could reveal things about the nature of habitability when it is the subject of follow-up observations using the James Webb Space Telescope (JWST).

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