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.

Oct 24, 2024 · TrES-3 b is a gas giant exoplanet that orbits a G-type star. Its mass is 1.91 Jupiters, it takes 1.3 days to complete one orbit of its star, and is 0.02282 AU from its star. Its discovery was announced in 2007.

Detailed information about planet TrES-3 b and its parameters. Planet-star interactions with precise transit timing. IV. Probing the regime of dynamical tides for GK host stars. Friends of Hot Jupiters. I. A Radial Velocity Search for Massive, Long-period Companions to …

CAMPAIGN: Planet included in one of the current observing campaings. TTVs: Planet exhibiting strong Trasit Time Variations due to another planet or orbital decay. ALERT: Observations in the last 2 years show an O-C greater than 10 minutes. HIGH: Prediction uncertainty greater than the target or less than 3 epochs observed in the last 2 years.

Oct 25, 2012 · TrES-3b, one of ∼282 1 confirmed transiting exoplanets, is a hot Jpiter orbiting a G-type star with a short orbital period of 1.306 19 ± 0.000 01 d, a mass of 1.92 ± 0.23 M Jup and a radius of 1.295 ± 0.081 R Jup (O'Donovan et al. 2007).

We observed nine primary transits of the hot Jpiter TrES-3b in several optical and near-UV photometric bands from 2009 June to 2012 April in an attempt to detect its magnetic field.

Aug 1, 2017 · The TrES-3b system, discovered by O’Donovan et al. (2007), consists of a slightly metal-poor G-type star with a mass of 0.9M ⊙ and a hot Jupiter with an orbital period of 1.3 days. In their study, analysis of both photometric and radial velocity data was presented.

May 31, 2020 · We present twelve new transit light curves of the hot-Jupiter TrES-3b observed during $2012-2018$ to probe the transit timing variation (TTV). By combining the mid-transit times determined from...

TrES-3b is an extrasolar planet orbiting the star GSC 03089-00929. It has an orbital period of just 31 hours and is undergoing orbital decay due to tidal effects. It has nearly twice the mass of Jupiter.

Apr 25, 2009 · TrES-3b gives a predicted 0.029 mag dimming. This measurement I measured a 0.022 mag dip based on the fitting done by Tresca--last time I was right on at 0.029.