Nasa-Forschungsteam entdeckt erstmals Atmosphäre auf Gesteins ...
Forscher der Nasa machen mit Studie bahnbrechende Entdeckung auf Exoplanet 55 Cancri e · Oberfläche aus Lava könnte Bildung einer sekundären ...
astronomy.com
Laut dem Fachportal <anchor>astronomy.com</anchor> scheint der „Planet trotz der heftigen Winde von seinem nahen Stern, der kontinuierlichen vulkanischen Aktivität und der Schwerkraft des Planeten eine relativ dichte Atmosphäre“ zu besitzen. „Bei diesen Temperaturen ist alles auf dem Planeten geschmolzen. Falls es sich um Gestein handelt, ist es geschmolzene Lava“, so Renyu Hu, Mitglied des Forschungsteams. Die Ausgasungsprozesse der geschmolzenen Oberfläche könnten die Bildung einer sekundären Atmosphäre begünstigt haben.
JWST finds a thick atmosphere around a rocky exoplanet, at last!
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at-last-jwst-finds-signs-of-a-thick-atmosphere-around-a-rocky-exoplanethttps://www.astronomy.com/science/at-last-jwst-finds-signs-of-a-thick-atmosphere-around-a-rocky-exoplanet/At last! JWST finds signs of a thick atmosphere around a rocky exoplanetAt last! JWST finds signs of a thick atmosphere around a rocky exoplanethttps://www.astronomy.com/uploads/2024/05/55-Cancri-e-exoplanet.jpegInStockUSD1.001.00exoplanetssciencearticleASY2024-07-242024-05-08145144

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# At last! JWST finds signs of a thick atmosphere around a rocky exoplanet

After coming up empty in other planetary systems, NASA’s flagship telescope has found the best evidence yet of a rich atmosphere around a rocky exoplanet.

By John Wenz |
Published: May 8, 2024 | Last updated on July 24, 2024

This is a color illustration of what exoplanet 55 Cancri e might look like. A rocky planet on the left and a portion of a much-larger star on the right. About three-quarters of the lit side of the planet is visible; the other quarter is in shadow. The surface of the planet has gray, orange, and yellow mottling. Most of the orange and yellow is in the region that is facing the star directly. The grayer portions are toward the poles and shadowed side of the planet. The edge of the disc of the planet appears to be glowing, suggesting a thin atmosphere. The star is bright orange-yellow, with a turbulent appearance similar to the Sun."

This is a NASA illustration from 2022 showing what exoplanet 55 Cancri e could look like. 55 Cancri e is a rocky planet with a diameter almost twice that of Earth orbiting just 0.015 astronomical units from its Sun-like star. Because of its tight orbit, the planet is extremely hot, with dayside temperatures reaching 4,400 degrees Fahrenheit (about 2,400 degrees Celsius). Credit: NASA.

It took a few attempts, but JWST has finally found strong evidence of an atmosphere around a rocky world outside our solar system. To add to the intrigue, this isn’t the planet’s original atmosphere — it’s a second atmosphere produced by volcanic activity. This history offers clues to how planets in otherwise inhospitable environments might be able to cling to habitable conditions.

The new observations, published May 8 in Nature, focus on the planet 55 Cancri e. It’s about twice the size of Earth and eight to nine times its mass. The planet is also likely covered in oceans of magma. It completes an orbit around its home star in about 17 hours — one of the fastest known orbital periods of any exoplanet. This leads to extreme conditions around its surface, with temperatures likely exceeding 3,000 degrees Fahrenheit — hot enough to melt most metals — and an intense bombardment of radiation from its host star.

As a result, the original atmosphere should be long gone. But by using JWST to measure the infrared light emitted by the planet, a team led by researchers at NASA’s Jet Propulsion Lab (JPL) in Pasadena, California, discovered the likely presence of carbon dioxide and carbon monoxide gas around the planet — marking the first time JWST has found strong signs of an atmosphere around a rocky planet.

The team also found no evidence for helium and hydrogen — the most common elements in the universe, which would have been part of the planet’s initial atmosphere when it formed. This means that the atmosphere detected is likely the planet’s secondary atmosphere. It seems that, despite the violent winds from its nearby star, continuous volcanic activity and the gravity of the planet have allowed the planet to remain enshrouded in a relatively thick atmosphere.

In short, 55 Cancri e shows that just because a planet loses its atmosphere, that doesn’t mean that it can’t gain a new one.

## Emission by subtraction

The study made use of a technique called secondary eclipse spectroscopy, which is possible when a planet’s orbit takes it behind its host star from our point of view. When the planet is eclipsed, astronomers can isolate the light coming from the host star and subtract it from observations of the full system, leaving behind the infrared light coming from the planet.

Though JWST’s suite of instruments includes a set of spectrometers, the atmospheric gasses weren’t detected by them directly. Instead, the astronomers behind the study looked at other properties of the atmosphere via the secondary eclipse, including its reflectivity. Then they ran simulations on a variety of possible atmospheric types that would give off similar signals.

The team found that the best match was a mix of carbon dioxide, carbon monoxide, and nitrogen gas. This would also track with a planetary atmosphere driven in part by volcanism.

This artist’s concept shows what the exoplanet 55 Cancri e could look like. Credit: NASA, ESA, CSA, Ralf Crawford (STScI). This artist’s concept shows what the exoplanet 55 Cancri e could look like. Credit: NASA, ESA, CSA, Ralf Crawford (STScI).

## A second chance at life?

To date, observations of Earth-like planets in the habitable zone of their stars have not yielded definitive detections of an atmosphere — their atmospheres have been mostly or completely stripped away by intense flares and the violent winds produced by their stars.

For instance, astronomers have come up empty using JWST to search for atmospheres around planets in the TRAPPIST-1 system. This system features seven Earth-sized planets, at least three of them in their host star’s habitable zone, where the surface temperature should allow water to be in liquid form.

While 55 Cancri e itself is not habitable, the possibility of secondary atmospheres developing on worlds that are could alter our understanding of how likely a planet is to support life.

“I’m quite confident that JWST will provide a lot of information about the ability of rocky planets of various sizes and temperatures to develop a secondary atmosphere,” says Renyu Hu, a planetary scientist at JPL and lead author of the paper. “We can use that to calibrate our models, and eventually, we will have a better understanding of the emergence of habitable worlds.”

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