Subscribe free to our newsletters via your
. 24/7 Space News .




EXO WORLDS
Hot, Super-Earths Help Track Water-Rich Atmospheres
by Nola Taylor Redd for Astrobiology Magazines
Moffett Field CA (SPX) Nov 26, 2014


The mass and radius of planets beyond the Solar System can be used to place some starting constraints on their atmospheres. If an observed planet has a larger radius than expected for a water-rich body, it would indicate that the planet has an atmosphere with a molecular composition lighter than water vapor, and might therefore be made up of elements such as hydrogen or helium, Madhusudhan said.

As the discovery of planets beyond the Solar System becomes more common, scientists have begun the in-depth study of the atmospheres of these bodies.

In a new paper, a pair of astronomers investigated the detectability of water in the atmospheres of far-away planets and found that hot, bright super-Earths are more easily identifiable with today's instruments than cooler ones.

Super-Earths are rocky bodies up to 10 times as massive as Earth, but not quite in the gas giant range. The compositions of these planets can range from solid rock to water-worlds atop a rocky crust.

Focusing on the hot version of super-Earths, which maintain water in vapor form rather than as a liquid on the surface, can provide insights into how much water could exist on cooler super-Earths.

Some of the cooler super-Earths have the potential to be habitable but their atmospheres are much more challenging to observe.

"We are interested in knowing how much water there is on super-Earths regardless of the phase - liquid or vapor," lead author Nikku Madhusudhan, of the University of Cambridge, told Astrobiology Magazine by email.

The research was published in a special exoplanet edition of the journal, The International Journal of Astrobiology.

Hotter planets, brighter futures
Madhusudhan and co-author Seth Redfield of Wesleyan University, in Connecticut, studied how qualities of an exoplanet that astronomers can observe, such as mass and radius, can help scientists narrow down what kind of atmosphere a planet could potentially have.

"Super-Earths are a mysterious class of planets because they seem to have a range of compositions, and also because we don't have any examples in the Solar System," planetary scientist Jacob Bean, of the University of Chicago, told Astrobiology Magazine.

Bean, who was not involved in the research, probes the atmospheres of super-Earths.

The mass and radius of planets beyond the Solar System can be used to place some starting constraints on their atmospheres. If an observed planet has a larger radius than expected for a water-rich body, it would indicate that the planet has an atmosphere with a molecular composition lighter than water vapor, and might therefore be made up of elements such as hydrogen or helium, Madhusudhan said.

Atmospheres represent a challenge to scientists, who struggle to observe the translucent outer layers of a planet. The passing starlight changes as it interacts with molecules in the atmosphere. By studying this light, known as spectra, scientists can identify the atmospheric composition. However, changes in the spectra are small compared to the overall light from the star, and require precision to study.

While the study of the atmospheres of larger gas giants, such as hot Jupiters, is in full swing, the smaller size of super-Earths makes their study more challenging. The smaller planets produce a smaller signal for scientists to study and identify.

The temperature of a planet, which primarily depends on how closely it orbits its star, also plays a role in our ability to detect its atmospheric composition. Scientists have a harder time detecting the atmosphere of a cooler planet than its warmer counterpart.

Characterizing the atmosphere of a super-Earth orbiting a star in its habitable zone (the region where liquid water could exist on the surface) is outside the abilities of today's instruments.

Future tools on upcoming telescopes, such as NASA's James Webb Space Telescope and the Thirty-Meter Telescope, which is expected to be the second-largest ground-based telescope when it sees first light around 2022, may be able to detect signatures in a few select cases, Madhusudhan said, but doing so will remain difficult.

As a result, the team focused on hot super-Earths with orbits on the order of days, particularly those traveling around hot, bright stars.

Only two hot super-Earths known today have good potential for atmospheric observations. 55 Cancri e boasts a temperature of over 3,100 degrees Fahrenheit (1,700 degrees Celsius) as it circles its star every 18 hours. Meanwhile, HD 97658 b travels around its star once every 9.5 days, reaching temperatures of about 1,100 degrees Fahrenheit (630 degrees C).

When it comes to detecting atmospheres, "clearly, 55 Cancri e is the ideal candidate at the moment," Madhusudhan said.

Many upcoming planet-finding surveys undertaken from space, such as TESS (Transiting Exoplanet Survey Satellite), CHEOPS (CHarcterising ExOPlanet Satellite), and PLATO (PLAnetary Transits and Oscillations of stars), as well as several ground-based surveys, are expected to find hundreds of such planets.

Cloudy skies
One reason close-orbiting super-Earths such as 55 Cancri e make better candidates to study is because their hot temperatures affect cloud formation. Although on Earth, clouds are made predominantly of water, at higher temperatures, clouds would form from heavier materials, such as iron and silicates. The cloud cover would settle lower to the ground, allowing more of the spectra of the atmosphere to pass through for scientists to identify.

Clouds lack the unique fingerprints that molecules present when scientists study their spectra, hindering the study of the atmosphere. For instance, GJ 1214b is a super-Earth orbiting a red dwarf star. Previous research suggested that this planet hosted a water-rich atmosphere, but Jacob Bean was part of a team that in 2013 detected clouds above the planet.

Another benefit of studying near-orbiting super-Earths is that they pass frequently between their star and our sun, allowing astronomers to gather more data over the same time scale than can be done with their cooler counterparts.

Studying hot super-Earths can help scientists understand more about super-Earths that lie in the habitable zone, even though the atmospheres of the cooler planets continue to elude detection.

Knowing how much water the hotter atmospheres contain can help constrain the amount of water on cooler planets, which should have formed from similar starting conditions that would have changed based on the planetary orbits.

"These calculations have helped sharpen our view of what information we can get from the spectra of super-Earths, and which individual objects are the best ones to focus our attention on," Bean said.


Thanks for being here;
We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain.

With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords.

Our news coverage takes time and effort to publish 365 days a year.

If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.

SpaceDaily Contributor
$5 Billed Once


credit card or paypal
SpaceDaily Monthly Supporter
$5 Billed Monthly


paypal only

.


Related Links
Astrobiology Magazine
Lands Beyond Beyond - extra solar planets - news and science
Life Beyond Earth






Comment on this article via your Facebook, Yahoo, AOL, Hotmail login.

Share this article via these popular social media networks
del.icio.usdel.icio.us DiggDigg RedditReddit GoogleGoogle




Memory Foam Mattress Review
Newsletters :: SpaceDaily :: SpaceWar :: TerraDaily :: Energy Daily
XML Feeds :: Space News :: Earth News :: War News :: Solar Energy News





EXO WORLDS
How to estimate the magnetic field of an exoplanet?
Moscow, Russia (SPX) Nov 24, 2014
Scientists developed a new method which allows to estimate the magnetic field of a distant exoplanet, i.e., a planet, which is located outside the Solar system and orbits a different star. Moreover, they managed to estimate the value of the magnetic moment of the planet HD 209458b. The group of scientists including one of the researchers of the Lomonosov Moscow State University (Russia) pu ... read more


EXO WORLDS
Young Volcanoes on the Moon

U.K. group to crowd-source funding for moon mission

After Mars, India space chief aims for the moon

China examines the three stages of lunar test run

EXO WORLDS
Within Rover's Reach at Mars Target Area 'Alexander Hills'

Mars Exploration Program Director Named

Second Time Through, Mars Rover Examines Chosen Rocks

Mars was warm enough for flowing water, but only briefly

EXO WORLDS
The International Space Station officially has an espresso machine

Astronauts to get 'ISSpresso' coffee machine

Tencent looks to the final travel frontier

ESA Commissions Airbus As contractor For Orion Service Module

EXO WORLDS
China expects to introduce space law around 2020

China launches new remote sensing satellite

China publishes Earth, Moon photos taken by lunar orbiter

China plans to launch about 120 applied satellites

EXO WORLDS
Soyuz docks at Space Station; Expedition 42 joins crew

Italy's first female astronaut heads to ISS in Russian craft

Space station gets zero-gravity 3-D printer

NASA Commercial Crew Partners Continue System Advancements

EXO WORLDS
Elon Musk unveils 'drone ship' and 'x-wing' fins for rockets via Twitter

Russian Rocket Supply for Satellites Launches Continues

China launches Yaogan-24 remote sensing satellite

Soyuz Installed at Baikonur, Expected to Launch Wednesday

EXO WORLDS
Hot, Super-Earths Help Track Water-Rich Atmospheres

How to estimate the magnetic field of an exoplanet?

Follow the Dust to Find Planets

NASA's TESS mission cleared for next development phase

EXO WORLDS
U.S. supplies Ukraine with counter-mortar radar systems

Versatile bonding for lightweight components

Cloaking device hides across continuous range of angles

A new approach to the delivery of satellites to orbit




The content herein, unless otherwise known to be public domain, are Copyright 1995-2014 - Space Media Network. All websites are published in Australia and are solely subject to Australian law and governed by Fair Use principals for news reporting and research purposes. AFP, UPI and IANS news wire stories are copyright Agence France-Presse, United Press International and Indo-Asia News Service. ESA news reports are copyright European Space Agency. All NASA sourced material is public domain. Additional copyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement, agreement or approval of any opinions, statements or information provided by Space Media Network on any Web page published or hosted by Space Media Network. Privacy Statement All images and articles appearing on Space Media Network have been edited or digitally altered in some way. Any requests to remove copyright material will be acted upon in a timely and appropriate manner. Any attempt to extort money from Space Media Network will be ignored and reported to Australian Law Enforcement Agencies as a potential case of financial fraud involving the use of a telephonic carriage device or postal service.