Earth's Cousins Orbiting a Distant Star

4 years ago Science

Corot_missionPhoto:
CoRot Mission
Artist - CNES / ESA

The Mission / The Star

The French Space Agency (CNES), in conjunction with the European Space Agency (ESA), launched the CoRoT (COnvection ROtation and planetary Transits) space mission on December 27, 2006. CoRoT's mission is searching for large terrestrial-like exoplanets that have short orbital periods. The mission has already confirmed seven new extraterrestrial planets, the latest of which is extraordinary and exciting. As a result, the CoRoT mission has been extended to January, 2010.

There are no Earth occultations to interfere with CoRoT’s telescope, a situation that allows for 150 days of continuous observation each year. CoRoT's small 27cm diameter telescope looks into the sky perpendicular to its orbital plane and detects small changes in the brightness of nearby stars. When an exoplanet moves across its sun’s spherical disc (transits), small changes occur in the star’s brightness which can be photographed and measured.

Earth-like planet / artistPhoto: IvoShandor / Wikimedia

CoRoT-7 is in the constellation of Monoceros, the Unicorn, on the celestial equator and is a main sequence orange dwarf. The surface temperature of CoRoT-7 is 5275K, its radius is 87% of the Sun, mass 93% of the Sun and metal abundance is approximately the same as that of our Sun. CoRoT-7 is 489 light years (150 parsecs) distant and 1.2–2.3 billion years old as compared to our Sun which is 4.6 billion years old. The seismic activity of CoRoT-7 makes observations by the CoRoT mission spacecraft a challenge.

CaRoT_7b_planetPhoto:
CaRoT_7b planet
Artist - ABC.es

The Planets

More than 330 exoplanets have been discovered, most of which are gas giants that resemble Jupiter, Saturn and Neptune. The CoRoT mission spacecraft has discovered two small planets orbiting the star CoRoT-7 that have an uncommon Earth-like structure. On February 3, 2009, CNES and ESA announced CoRoT's discovery of the smallest terrestrial planet ever found, the first of these two unusual planets that are in orbit around the star CoRoT-7.

CoRoT-7b is less than twice the size of the Earth with a mass 5.0X Earth and it is the first Super Earth planet found whose radius can be measured. It is located very close to its parent star and completes an orbit in 20 hours which is the shortest orbital period of any known planet. CoRoT-7b was discovered when it transited CoRoT-7 and caused a dimming of its star’s light until the transit was completed. The star and this planet exchange strong tidal forces.

CoRoT-7b planetPhoto:
CoRoT-7b planet
Artist - telescop.ucoz

CoRoT-7b has a high surface temperature between 1000°C and 1500°C and there are several possibilities for its surface composition. If no atmosphere is assumed, the irradiated face of CoRoT-7b might be 1800°K–2000°K; and the dark hemisphere could be as cold as 50°K. CoRot-7b might be covered in lava or water vapor; or have a predominantly rocky Earth-like surface; or have water and rock in equal amounts. If CoRot-7b becomes the first confirmed ocean planet, it would be covered in a great sea that formed when an icy surface melted as the planet drifted towards its star and the surface temperature rose. Yet another possibility is that CoRot-7B is a Chthonian Planet that initially resembled Neptune, but then lost a great deal of mass because of close proximity to the massive gravitational pull of CoRoT-7.

Media reports that CoRoT-7b has been confirmed as unambiguously ‘rocky’ as is the Earth are not quite accurate. There are several options for surface morphology. With a terrestrial density comparable to Earth, Mercury, Mars and Venus, there is an exciting possibility that CoRot-7b has a surface on which there are large, rocky land masses amidst one or more oceans.

CoRoT-7_b_planetPhoto:
CoRoT-7 b planet
Artist - exoplanetz

The first detailed information about CoRoT-7c – the second Super Earth planet in orbit around CoRoT-7 – was published in late August, 2009. Data was contributed by international partners at the European Southern Observatory at Paranal, the 3.6 meter telescope at La Silla (Chile) and the Euler Swiss telescope. The mass of CoRoT-7c is ~8.0X Earth, and its density is similar to that of Earth. The planet’s surface may also be composed of water, ice and rocks.

The star CoRoT-7 is the brightest star known with transiting planets. CoRoT-7 is also the first star discovered with a planetary system composed of two short period, Super Earth mass planets with one in transit. Super Earth planets have the closest resemblances to Earth of all the extraterrestrial planets. These discoveries hint at exciting possibilities for the existence of cellular life elsewhere in the galaxy!

Sources: 1, 2, 3

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Copyright(c) Blumenberg Associates LLC, 2010. This article may be posted and copied elsewhere on blogs and in not-for-profit contexts with the requirement that this copyright notice is clearly visible. For use in for-profit business, please contact the author.

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merlynne6 says

Jun 17th, 2010 at 12am
On June 16, 2010, the CNES CoRoT mission and space telescope announced several important exoplanet discoveries. CoRoT-8b is small, about 70% the size and mass of Saturn and is expected to have a structure similar to ice-giant planets like Uranus and Neptune. CoRoT-10b has an extremely elongated orbit with a year of 13 earth days. Radiation received from its star varies 10X and surface temperature varies from 250 to 600°C. CoRoT-11b orbits a very rapidly rotating star that rotates about its axis in 40 hours. CoRoT 12b, 13b and 14b are large exoplanets. CoRoT 12b is a 'bloated hot Jupiter' that is expected to have a rocky core. CoRoT 13b is smaller than Jupiter but 2X dense. CoRoT-14b is similar in size to Jupiter, 7.5X as massive, and only the second massive planet of this type discovered. Visit: http://www.physorg.com/news195720221.html for more information