Saturday, November 28, 2015

Blue skied neptune size exoplanet around red dwarf GB 3470b that is 100 light years away

http://ift.tt/hZ0OVi
A team of astronomers have used the LCOGT network to detect light scattered by tiny particles (called Rayleigh scattering), through the atmosphere of a Neptune-size transiting exoplanet. This suggests a blue sky on this world which is only 100 light years away from us. The result was published in the Astrophysical Journal on November 20 (and is available on ArXiV).

They observed several transits of GJ 3470b, a warm Neptune analog around an early M dwarf, in four different bands with the LCOGT and Kuiper telescopes.

Transits occur when an exoplanet passes in front of its parent star, reducing the amount of light we receive from the star by a small fraction. When the orbit of an exoplanet is aligned just right for transits to occur, astronomers can measure the planet’s size at different wavelengths in order to generate a spectrum of its atmosphere. The spectrum then reveals the substances present in the planet’s atmosphere, and therefore its composition. This measurement is most often performed using infrared light, where the planet is brightest and most easily observed. During the last few years, researchers have been probing the atmospheres of several small exoplanets with large ground and space-based telescopes, but have found it challenging to determine their composition using this method. This is either because the planets have clouds (which obscure the atmosphere) or because the measurements were not sufficiently precise.

At four times the size of the Earth, GJ 3470b is a transiting exoplanet closer in size to our own planet than to the hot Jupiters (about 10 times the size of the Earth) which so far make up the majority of exoplanets with well-characterized atmospheres. Astronomers led by Diana Dragomir of the University of Chicago have followed up on a discovery by a different group, whose results tentatively hinted at the presence of Rayleigh scattering in the atmosphere of GJ 3470b. Dr. Dragomir’s team acquired and combined transit observations from all of LCOGT’s observatory sites (Hawaii, Texas, Chile, Australia and South Africa) to conclusively confirm the detection of Rayleigh scattering for GJ 3470b.




Arxiv - Rayleigh Scattering in the Atmosphere of the Warm Exo-Neptune GJ 3470b

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Reposted via Next Big Future

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