GSC 03549-02811 explained

GSC 03549-02811 (sometimes referred to as Kepler-1, or either TrES-2A or TrES-2 parent star in reference to its exoplanet TrES-2b)[1] is a binary star containing a yellow main-sequence star similar to the Sun. This star is located approximately 750 light-years away in the constellation of Draco. The apparent magnitude of this star is 11.41, which means it is not visible to the naked eye but can be seen with a medium-sized amateur telescope on a clear dark night. The age of this star is about 5 billion years.[2]

Planetary system

In 2006 the exoplanet TrES-2b was discovered by the TrES program using the transit method. It is also within the field of view of the previously operational Kepler Mission planet-hunter spacecraft. This system continues to be studied by other projects and the parameters are continuously improved.[3] The planet orbits the primary star.

Though TrES-2b is currently the darkest known exoplanet, reflecting less than 1 percent of local sunlight, it shows a faint red glow. This is because its surface is 1,100 °C, it is so hot that it glows red. It is assumed to be tidally locked to its parent star.[4]

Binary star

In 2008 a study was undertaken of fourteen stars with exoplanets that were originally discovered using the transit method through relatively small telescopes. These systems were re-examined with the 2.2M reflector telescope at the Calar Alto Observatory in Spain. This star system, along with two others, was determined to be a previously unknown binary star system. The previously unknown secondary star is a dim magnitude 15 K-type star separated by about 232 AU from the primary, appearing offset from the primary by about one arc second in the images. This discovery resulted in a significant recalculation of parameters for both the planet and the primary star.

The Kepler mission

See main article: Kepler space telescope.

In March 2009 NASA launched the Kepler spacecraft. This spacecraft was a dedicated mission to discover extrasolar planets by the transit method from solar orbit. In April 2009 the project released the first light images from the spacecraft and TrES-2b was one of two objects highlighted in these images. Although TrES-2b is not the only known exoplanet in the field of view of this spacecraft it is the only one identified in the first-light images. This object is important for calibration and check-out.[5]

See also

External links

Notes and References

  1. D. Mislis . S. Schroter . J.H.M.M. Schmitt . O. Cordes . K. Reif . 0912.4428v1 . Multi-band transit observations of the TrES-2b exoplanet . astro-ph.EP. December 2009 .
  2. Kepler-1 . 2009-04-22 .
  3. Improving Stellar and Planetary Parameters of Transiting Planet Systems: The Case of TrES-2. The Astrophysical Journal. Alessandro Sozzetti. August 1, 2007 . 664. 2. 1190–1198. 10.1086/519214. 2007ApJ...664.1190S. 0704.2938 . Torres. Guillermo. Charbonneau. David. Latham. David W.. Holman. Matthew J.. Winn. Joshua N.. Laird. John B.. o’Donovan. Francis T.. 17078552.
  4. Web site: Coal-Black Alien Planet is Darkest Ever Seen. 11 August 2011 .
  5. Web site: Kepler Eyes Cluster and Known Planet. NASA. 2009-04-16. 2009-05-09.