|Extrasolar planet||List of extrasolar planets|
|Star||GSC 03549-02811 A|
|Right ascension||(α)||19h 07m 14.035s|
|Declination||(δ)||+49° 18′ 59.07″|
|Semimajor axis||(a)||0.03556±0.00075 AU|
|Orbital period||(P)||2.47063±0.00001 d|
|Bond Albedo||(%)||0.04 %|
|Surface gravity||(g)||3.284±0.016 g|
|Discovery date||August 21, 2006
confirmed September 8, 2006
|Discoverer(s)||O'Donovan et al.|
|Other detection methods||Radial velocity,
Orbital light variations
|Discovery site||California & Arizona|
TrES-2b (or Kepler-1b) is an extrasolar planet orbiting the star GSC 03549-02811 located 750 light years away from our solar system. The planet has been identified in 2011 as the darkest known exoplanet, reflecting less than 1% of any light that hits it. The planet's mass and radius indicate that it is a gas giant with a bulk composition similar to that of Jupiter. Unlike Jupiter, but similar to many planets detected around other stars, TrES-2b is located very close to its star, and belongs to the class of planets known as hot Jupiters. This system was within the field of view of the now nonoperational Kepler spacecraft.
This planet continues to be studied by other projects and the parameters are being improved continuously. A 2007 study improved stellar and planetary parameters. A 2008 study concluded that the TrES-2 system is a binary star system. This has a significant effect on the values for the stellar and the planetary parameters.
TrES-2b was discovered on August 21, 2006 by the Trans-Atlantic Exoplanet Survey (TrES) by detecting the transit of the planet across its parent star using Sleuth (Palomar Observatory, California) and PSST (Lowell Observatory, Arizona), part of the TrES network of 10–cm telescopes. The discovery was confirmed by the W. M. Keck Observatory on September 8, 2006, by measuring the radial velocity of the star that hosts TrES-2b.
In August 2008 more details of the relationship between the parent star and the orbit of the planet were published. The orbit was determined to be tilted by −9±12° from the stellar equator. The orbital direction was determined to be in the same direction as the star's rotation (prograde).
The Kepler mission
NASA launched Kepler in March 2009. The spacecraft is dedicated to the discovery of 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.
The first important result from the Kepler Mission about TrES-2b is an extremely low geometric albedo, measured in 2011. If the entire day-night contrast were due to geometric albedo, it would be 2.53%, but modeling suggests that much of this is dayside emission and the true albedo is much lower. It is estimated to be less than 1% and for best-fit model it is about 0.04%. This makes TrES-2b the darkest known exoplanet, reflecting less light than coal or black acrylic paint. It is not clear why the planet is so dark. One reason could be an absence of reflective clouds such as those which make Jupiter so bright, due to TrES-2b's proximity to its parent star and the consequent high temperature. Another reason could be the presence in the atmosphere of light-absorbing chemicals such as vaporized sodium, potassium, or gaseous titanium oxide. In general, hot Jupiters are expected to be dark, because "absorption due to the broad wings of the sodium and potassium D lines is thought to dominate their visible spectra." Apart from that of Kepler-7b (38±12%), albedo measurements for hot Jupiters have generally given only upper limits.
- Daemgen, S.; Hormuth, F.; Brandner, W.; Bergfors, C.; Janson, M.; Hippler, S.; Henning, T. (2009). "Binarity of transit host stars — Implications for planetary parameters" (PDF). Astronomy and Astrophysics 498 (2): 567–574. arXiv:0902.2179. Bibcode:2009A&A...498..567D. doi:10.1051/0004-6361/200810988.
- David M. Kipping & David S. Spiegel. "Detection of visible light from the darkest world". Monthly Notices of the Royal Astronomical Society. Retrieved 2011-08-12.
- O'Donovan, Francis T.; Charbonneau, David; Mandushev, Georgi; Dunham, Edward W.; Latham, David W.; Torres, Guillermo; Sozzetti, Alessandro; Brown, Timothy M. et al. (2006). "TrES-2: The First Transiting Planet in the Kepler Field". The Astrophysical Journal Letters 651 (1): L61–L64. arXiv:astro-ph/0609335. Bibcode:2006ApJ...651L..61O. doi:10.1086/509123.
- Alessandro Sozzetti et al. (August 1, 2007). "Improving Stellar and Planetary Parameters of Transiting Planet Systems: The Case of TrES-2". The Astrophysical Journal 664 (2): 1190–1198. arXiv:0704.2938. Bibcode:2007ApJ...664.1190S. doi:10.1086/519214.
- Winn, Joshua N.; Johnson, John Asher; Narita, Norio; Suto, Yasushi; Turner, Edwin L.; Fischer, Debra A.; Butler, R. Paul; Vogt, Steven S. et al. (2008). "The Prograde Orbit of Exoplanet TrES-2b". The Astrophysical Journal 682 (2): 1283–1288. arXiv:0804.2259. Bibcode:2008ApJ...682.1283W. doi:10.1086/589235.
- "Kepler Eyes Cluster and Known Planet". NASA. 2009-04-16. Retrieved 2009-05-09.
- "Coal-Black Alien Planet Is Darkest Ever Seen". Space.com. Retrieved 2011-08-12.
- Baldwin, Emily (2011-08-11). "Exoplanet blacker than coal". Astronomy Now. Retrieved 2011-08-12.
|Wikimedia Commons has media related to TrES-2b.|
- Host to 'Hot Jupiter' (labeled) NASA, 2009-04-16
- TrES-2: Most Massive Nearby Transiting Exoplanet
- Jupiter-Sized Transiting Planet Found by Astronomers Using Novel Telescope Network
- Light curve for TrES-2b using differential photometry