This Exoplanet is Probably a Solid Ball of Metal

An illustration of the exoplanet Gliese 367 b. It's an oddball planet that may be composed entirely of iron. Image Credit: NASA

We can’t understand nature without understanding its range. That’s apparent in exoplanet science and in our theories of planetary formation. Nature’s outliers and oddballs put pressure on our models and motivate scientists to dig deeper.

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An Ambitious New Technology Might be Needed to See Other Earths

How a starshade would reveal exoplanets. Credit: NASA/JPL

The race is on to discover truly habitable Earth-like worlds. While we are starting to observe the atmospheres of large potentially habitable planets such as Hycean worlds with the telescopes we currently have, the most significant breakthroughs will likely come with the development of advanced specialized telescopes. These new designs will likely use a starshade to hide the glare of a star and allow us to directly observe its exoplanets. But will that be enough to study distant terrestrial planets?

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If Astronomers See These Chemicals in a Planet’s Atmosphere, There’s Likely an Advanced Civilization There

Artist rendition of a potential water-world exoplanet that might support advanced civilizations. Such life could advertise its existence via technosignatures from industrial or other activities. (Credit: ESA / Hubble / M. Kornmesser)
Artist rendition of a potential water-world exoplanet that might support life. Scientists could determine whether to explore this world based on its planetary entropy production. (Credit: ESA / Hubble / M. Kornmesser)

In an age of ever-growing numbers of exoplanets circling other stars, it’s natural that astronomers search for signatures of advanced civilizations. Such signatures may have biological or technological origins.

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Planning is Underway for NASA’s Next Big Flagship Space Telescope

Artist rendition of a starshade being used on a future space telescope. This example shows the proposed Habitable Exoplanet Observatory (HabEx), which the 2020 Astrophysics Decadal Survey decided to combine elements of this with the Large Ultraviolet Optical Infrared Surveyor (LUVOIR) for a new flagship telescope, which is now known as the Habitable Worlds Observatory (HWO). (Credit: NASA)

NASA’s James Webb Space Telescope (JWST) has only been operational for just over a year, but this isn’t stopping the world’s biggest space agency from discussing the next big space telescope that could serve as JWST’s successor sometime in the future. Enter the Habitable Worlds Observatory (HWO), which was first proposed as NASA’s next flagship Astrophysics mission during the National Academy of Sciences’ Decadal Survey on Astronomy and Astrophysics 2020 (Astro2020). While its potential technological capabilities include studying exoplanets, stars, galaxies, and a myriad of other celestial objects for life beyond Earth, there’s a long way to go before HWO will be wowing both scientists and the public with breathtaking images and new datasets.

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Do The Gaps in Protoplanetary Disks Really Indicate Newly Forming Planets?

Artist depiction of a protoplanetary disk in which planets are forming. Credit: ESO/L. Calçada

Roughly 5 billion years ago Earth was in the process of forming. Gas and dust gathered with the young Sun’s protoplanetary disk, likely nudged a bit by the resonant gravitational pull of Jupiter and other large worlds. One can imagine that as Earth formed it swept its orbit clear of debris, leaving a gap in the disk visible from light years away. While we know this tale is reasonably accurate, the idea that planets such as Earth always clear gaps in a protoplanetary disk likely isn’t.

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JWST Might Have Imaged a Hycean World for the First Time, With a Hydrogen-Rich Atmosphere and a Deep Planet-Wide Water Ocean

Artist depiction of the mini-Neptune K2-18 b. Credit: NASA, CSA, ESA, J. Olmstead (STScI), N. Madhusudhan (Cambridge University)

Despite its great oceans, Earth is not really an ocean world. It has less water than icy moons such as Europa and Enceladus, a relatively thin nitrogen-rich atmosphere, and vast continents that rise above sea level. A true ocean world would have no continents, a warm sea hundreds of kilometers deep, and a thick hydrogen and water-rich atmosphere. They are known as hydrogen-ocean planets or hycean worlds. While we’ve long thought they exist, the James Webb Space Telescope may now have found one.

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TESS Finds a Planet That Takes 482 Days to Orbit, the Widest it’s Seen so Far

An artist's rendition of the two planets and star in the TOI-4600 system. One of them has the longest orbit of any planet yet found by TESS. Image Credit: Tedi Vick

We’re rapidly learning that our Solar System, so familiar to us all, does not represent normal.

A couple of decades ago, we knew very little about other solar systems. Astronomers had discovered only a handful of exoplanets, especially around pulsars. But that all changed in the last few years.

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Astronomers Confirm First Exoplanet “Thermometer Molecule” that is Typically Used to Study Brown Dwarfs

Artist impression of "hot Jupiter" exoplanet, WASP-31 b. (Credit: ESA/Hubble & NASA)

A recent study published in The Astrophysical Journal Letters examines a rare alloy molecule known as chromium hydride (CrH) and its first-time confirmation on an exoplanet, in this case, WASP-31 b. Traditionally, CrH is only found in large quantities between 1,200 to 2,000 degrees Kelvin (926.85 to 1,726.85 degrees Celsius/1700 to 3,140 degrees Fahrenheit) and used to ascertain the temperature of cool stars and brown dwarfs. Therefore, astronomers like Dr. Laura Flagg in the Department of Astronomy and Carl Sagan Institute at Cornell University refer to CrH as a “thermometer for stars”.

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A Neptune-sized Exoplanet is Denser Than Steel. The Result of a Catastrophic Collision?

An artist's conception of a hot Neptune. TOI-1538b is a super-dense version of this type of exoplanet and its core is denser than steel. Courtesy Pablo Carlos Budassi, CC BY-SA 4.0.
An artist's conception of a hot Neptune. TOI-1538b is a super-dense version of this type of exoplanet and its core is denser than steel. Courtesy Pablo Carlos Budassi, CC BY-SA 4.0.

There’s an odd exoplanet out there posing a challenge to planetary scientists. It’s a hot Neptune denser than steel. The big question is: how did it form?

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Watch an Actual Exoplanet Orbit its Star for 17 Years

Artist rendition of exoplanet, Beta Pictoris b, whose partial orbit was recently featured in a time-lapsed video. (Credit: ESO L. Calçada/N. Risinger)

Searching for exoplanets is incredibly difficult given their literal astronomical distances from Earth, which is why a myriad of methods have been created to find them. These include transit, redial velocity, astrometry, gravitational microlensing, and direct imaging. It is this last method that was used to recently create a time-lapse video that compresses a mind-blowing 17 years of the partial orbit of exoplanet, Beta Pictoris b, into 10 seconds. The data to create the video was collected between 2003 and 2020, it encompasses approximately 75 percent of the total orbit, and marks the longest time-lapse video of an exoplanet ever produced.

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