From Surf Wiki (app.surf) — the open knowledge base
TrES-3b
Hot Jupiter
Hot Jupiter
| Field | Value | |
|---|---|---|
| name | TrES-3b / Umbäässa | |
| image | Exoplanet Comparison TrES-3 b.png | |
| caption | Size comparison of TrES-3b with Jupiter. | |
| <!-- DISCOVERY --> | discoverer | O'Donovan et al. |
| discovery_site | United States | |
| discovered | 2007 | |
| discovery_method | Transit | |
| <!-- ORBITAL --> | apsis | astron |
| semimajor | 0.0226 ± | |
| period | 1.30619 ± 0.00005 d | |
| inclination | 82.15 | |
| star | GSC 03089-00929 | |
| <!-- PHYS CHARS --> | mean_radius | 1.341 ± 0.081 |
| mass | 1.92 ± 0.23 | |
| density | 1172 kg/m3 | |
| surface_grav | 2.7 g | |
| single_temperature | 1555 K |
TrES-3b is an extrasolar planet orbiting the star GSC 03089-00929. It has an orbital period of just 31 hours and nearly twice the mass of Jupiter.
The planet TrES-3b is named Umbäässa. The name was selected in the NameExoWorlds campaign by Liechtenstein, during the 100th anniversary of the IAU. In the local dialect of southern Liechtenstein, Umbäässa is a small and barely visible ant.
Discovery
It is the third transiting planet found by the Trans-Atlantic Exoplanet Survey. It was discovered in the constellation Hercules about 10 degrees west of Vega, the brightest star in the summer skies.
Transits in front of the star GSC 03089-00929 were detected by two 10 cm telescopes operating out of Palomar and Lowell Observatories. Transits of TrES-3 were also independently observed by the Hungarian Automated Telescope Network. Seven high-precision radial velocity measurements were made using the HIRES spectrometer at W. M. Keck Observatory, which confirmed the presence of a planetary mass companion with a minimum mass twice that of the planet Jupiter.
Characteristics
The planet's home star is slightly smaller and cooler than the Sun. The orbital period is less than one and a third days, one of the shortest known. Despite close proximity to the star, no evidence of tidal-driven orbital decay was present as in 2020, with best data fit indicating only an apsidal precession of planetary orbit.
References
References
- (2020). "Multi-color photometry and parameters estimation of Jupiter-sized exoplanets; TRES-3b, WASP-2b and HATP-30b".
- "Approved names".
- "International Astronomical Union {{!}} IAU".
- (2020). "Probing Transit Timing Variation and Its Possible Origin with 12 New Transits of TrES-3b". The Astronomical Journal.
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
Ask Mako anything about TrES-3b — get instant answers, deeper analysis, and related topics.
Research with MakoFree with your Surf account
Create a free account to save articles, ask Mako questions, and organize your research.
Sign up freeThis content may have been generated or modified by AI. CloudSurf Software LLC is not responsible for the accuracy, completeness, or reliability of AI-generated content. Always verify important information from primary sources.
Report