Click here to sign in with

or

Forget Password?

Learn more

October 26, 2020

by University of New Mexico

An international team of scientists recently measured the spectrum of the atmosphere of a rare hot Neptune exoplanet, whose discovery by NASA’s Transiting Exoplanet Survey Satellite (TESS) was announced just last month.

googletag.cmd.push(function() { googletag.display(‘div-gpt-ad-1449240174198-2’); });

The discovery was made with data provided from the now-retired NASA Spitzer Space Telescope, which allows a unique, infrared view of the universe to look into regions of space that are hidden from optical telescopes.

One of the main goals of NASA’s TESS mission is to find new, small planets that would be good targets for atmospheric characterization. Early in its mission, it found LTT9779b, a planet orbiting a Sun-like star located 260 light years away from Earth. This planet, a little larger than Neptune, orbits very close to its star. The planet is found in thehot Neptune desert,” where planets shouldn’t exist. Indeed, most close-in hot exoplanets are either gas giants the size of Jupiter or Saturn that have enough mass to retain most of their atmosphere using their high gravity against the evaporation caused by the star, or small rocky exoplanets that have lost their atmosphere to the star long ago.

This ultra-hot Neptune is a ‘medium-sizedexoplanet that orbits very close to its star (it takes just 19 hours to complete an orbit), but its low density indicates that it still has an atmosphere weighing at least 10 percent of the planet’s mass,” explained University of New Mexico Physics and Astronomy Assistant Professor Diana Dragomir, who is leading the work which involved more than 25 institutions.

The age of this system is 2 billion years. At this high temperature, the planet’s atmosphere should have evaporated long ago, early in the system’s life. “Hot Neptunes are rare, and one in such an extreme environment as this one is difficult to explain because its mass isn’t large enough to hold on to an atmosphere for very long. So how did it manage? LTT9779b had us scratching our heads, but the fact that it has an atmosphere gives us a rare way to investigate this type of planet, so we decided to probe it with another telescope,” Dragomir added.

To investigate its atmospheric composition and shed further light on its origin, scientists obtained secondary eclipse observations with the Spitzer Infrared Array Camera (IRAC) of the hot Neptune. The Spitzer observations confirmed an atmospheric presence and enabled a measurement of the planet’s very high temperature, approximately 2,000 Kelvin (about 3,000 degrees Fahrenheit). “For the first time, we measured light coming from a planet that shouldn’t exist!” Said Dragomir.

After combining the Spitzer observations with a measurement of the secondary eclipse in the TESS bandpass, the scientists studied the resulting emission spectrum and identified evidence of molecular absorption in the planet’s atmosphere, which they believe is likely due to carbon monoxide. This molecule is not unexpected in the atmospheres of hot large planets (hot Jupiters), but to find it in a hot Neptune may provide clues on the origin of this planet and how it managed to hold onto its atmosphere. This result constitutes the first detection of atmospheric features in an exoplanet discovered by TESS, and the first-ever for an ultra-hot Neptune.

If there’s a lot of atmosphere surrounding the planet, as is the case for LTT9779b, then you can study it more easily,” said Dragomir. “A smaller atmosphere would be much harder to observe.The results indicate that LTT9779b is an excellent target for additional characterization with NASA’s upcoming James Webb Space Telescope (JWST), which could also verify whether the observed molecular absorption is indeed due to carbon monoxide.

A companion paper, led by Kansas University Assistant Professor Ian Crossfield, also found signs that point to the planet’s atmosphere having a higher level of heavy elements than expected. This is additionally intriguing because the two similarly-sized planets in our Solar System, Neptune and Uranus, are primarily composed of light elements like hydrogen and helium.

LTT9779 is one of those super-exciting targets, a very rare gemstone for our understanding of hot Neptunes. We believe we detected carbon-monoxide in its atmosphere and that the permanent dayside is very hot, while very little heat is transported to the night side,” said Björn Benneke, professor at Université de Montréal and member of the Institute for Research on exoplanets (iREx). “Both findings make LTT9779b say that there is a very strong signal to be observed making the planet a very intriguing target for future detailed characterization with JWST.

Together, these results set the stage for similar investigations of a larger sample of exoplanets discovered in this hot Neptune desert, which are key to uncovering the origin of this unique population of exoplanets.

The research, Spitzer Reveals Evidence of Molecular Absorption in the Atmosphere of the Hot Neptune LTT 9779b, was published in The Astrophysical Journal Letters.

Thank you for taking your time to send in your valued opinion to Science X editors.

You can be assured our editors closely monitor every feedback sent and will take appropriate actions. Your opinions are important to us.

We do not guarantee individual replies due to extremely high volume of correspondence.

Your email address is used only to let the recipient know who sent the email. Neither your address nor the recipient’s address will be used for any other purpose.
The information you enter will appear in your e-mail message and is not retained by Phys.org in any form.

Get weekly and/or daily updates delivered to your inbox.
You can unsubscribe at any time and we’ll never share your details to third parties.

This site uses cookies to assist with navigation, analyse your use of our services, and provide content from third parties.
By using our site, you acknowledge that you have read and understand our Privacy Policy
and Terms of Use.

Source: https://phys.org/news/2020-10-reveals-evidence-molecular-absorption-atmosphere.html

Exoplanet, Hot Neptune, Atmosphere, Earth, Star, Molecule, Research

World news – US – Data reveals evidence of molecular absorption in the atmosphere of a hot Neptune

Building on its expertise in the areas of digital, technologies and processes , CSS Engineering you in your most ambitious transformation projects and helps you bring out new ideas, new offers, new modes of collaboration, new ways of producing and selling.

CSS Engineering is involved in projects each customer as if it were his own. We believe a consulting company should be more than an advisor. We put ourselves in the place of our customers, to align we incentives to their goals, and collaborate to unlock the full potential their business. This establishes deep relationships and enjoyable.

Our services:

  1. Create professional websites
  2. Hosting high performance and unlimited
  3. Sale and video surveillance cameras installation
  4. Sale and Installation of security system and alarm
  5. E-Marketing

All our achievements here https://www.css-engineering.com/en/works/

LEAVE A REPLY

Please enter your comment!
Please enter your name here