GSC 03549-02811

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GSC 03549-02811
Kepler First Light Detail TrES-2.jpg
GSC 03549-02811 and TrES-2b as seen from the Kepler spacecraft. Celestial north is to the left.
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Draco
A
Right ascension 19h 07m 14.035s[1]
Declination +49° 18′ 59.07″[1]
Apparent magnitude (V) 11.41
B
Right ascension ~19h 07m 14s[2]
Declination ~+49° 18′ 59″[2]
Apparent magnitude (V) 14.73[2]
Characteristics
Spectral type G0V[1]/K[2]
Apparent magnitude (B) ~12.030[1]
Apparent magnitude (V) 11.411±0.005[1]
Apparent magnitude (J) 10.232±0.020[1]
Apparent magnitude (H) 9.920±0.026[1]
Apparent magnitude (K) 9.846±0.022[1]
Astrometry
Proper motion (μ) RA: 2.9[1] mas/yr
Dec.: -3.4[1] mas/yr
Distance 718±33 ly
(220±10 pc)
Details
Mass 1.05[2]/0.67[2] M
Radius 1.000+0.036
−0.033
[3] R
Temperature 5850±50[3] K
Metallicity −0.15±0.1[3]
Age 5.1+2.7
−2.3
×109
[3] years
Other designations
TrES-2 A, KIC 11446443, KOI 1, 2MASS J19071403+4918590, TYC 3549-2811-1[1]
Database references
SIMBAD data
Extrasolar Planets
Encyclopaedia
data

GSC 03549-02811 A (referred to as TrES-2 or TrES-2 A in reference to its exoplanet)[4] is a yellow main-sequence star similar to our Sun. This star is located approximately 718 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.[1]

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.[5] This system continues to be studied by other projects and the parameters are continuously improved.[3] The planet orbits the primary star.[2]

The GSC 03549-02811 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
TrES-2b 1.199±0.052[2] MJ 0.03556±0.00075[2] 2.47063±0.00001[5] 0 1.272 RJ

Though TrES-2b is currently the darkest known exoplanet, reflecting less than 1 percent of local sunlight, it does show a faint red glow. This is because its surface is a punishing 1,100'C, so hot that it actually glows red. It is assumed to be tidally locked to its parent star.[6]

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.[2]

The Kepler Mission

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An image from Kepler with TrES-2b and another point of interest outlined. Celestial north is towards the lower left corner.

In March 2009 NASA launched the Kepler Mission spacecraft. This spacecraft is 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.[7]

See also

References

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  2. 2.0 2.1 2.2 2.3 2.4 2.5 2.6 2.7 2.8 2.9 Lua error in package.lua at line 80: module 'strict' not found.
  3. 3.0 3.1 3.2 3.3 3.4 Lua error in package.lua at line 80: module 'strict' not found.
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  6. http://news.yahoo.com/coal-black-alien-planet-darkest-ever-seen-220601419.html
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External links

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Coordinates: Sky map 19h 07m 14s, +49° 18′ 59″