TrES-4
Exoplanet TrES-4 |
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Size comparison between Jupiter (left) and TrES-4 (computer graphics) | |
Constellation | Hercules |
Position equinox : J2000.0 |
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Right ascension | 17h 53m 13s |
declination | + 37 ° 12 ′ 42 ″ |
Orbit data | |
Central star | GSC 02620-00648 |
Major semi-axis | (0.0509 ± 0.0007) AE |
Period of circulation | 3.5539 days |
Further data | |
diameter | approx. 244,000 km |
Dimensions | (0.92 ± 0.07) M J |
distance | 1400 ly (440 ± 60) pc |
history | |
discovery | TrES , Mandushev et al. |
Date of discovery | 2007 |
Catalog names | |
TrES-4 | |
More information | |
Hot Jupiter |
TrES-4 , also called TrES-4 b , is an exoplanet in the constellation Hercules and about 440 parsecs (approx. 1,400 ly ) from Earth . It consists mainly of hydrogen and has an extremely low density . TrES-4 orbits the star GSC 02620-00648 with an orbital period of 3.55 days .
Physical Properties
TrES-4 has 1.704 times the diameter of Jupiter (this corresponds to approx. 244,000 km), but has only about 92 percent of its mass (1.75 · 10 27 kg). Its average density is around 0.33 grams per cubic centimeter and well below that of Jupiter. Due to its close proximity to the central star - the distance is around 7.5 million kilometers (0.05 AU ) - the planet has a surface temperature of around 1,600 Kelvin .
Theoretical problem
TrES-4 poses a theoretical problem. According to the Lowell Observatory, the planet is much too big for a gas planet , measured by its mass and temperature. The cause of this fact has not yet been clarified.
See also
Individual evidence
Web links
- Largest Transiting Extrasolar Planet Found Around A Distant Star - Article at Lowell Observatory Media Room
- TrES-4 (English) - Entry at Extrasolar Planets Encyclopaedia
- TrES-4 b - Entry on Planet.ch