
TrES-1b - Wikipedia
TrES-1b is an extrasolar planet approximately 523 light-years away in the constellation of Lyra (the Lyre). The planet's mass and radius indicate that it is a Jovian planet with a similar bulk …
TrES-1 b - Science@NASA
Mar 28, 2025 · TrES-1 b is a gas giant exoplanet that orbits a K-type star. Its mass is 0.84 Jupiters, it takes 3 days to complete one orbit of its star, and is 0.03925 AU from its star. Its …
GSC 02652-01324 - Wikipedia
GSC 02652-01324, also known as V672 Lyrae, is an orange dwarf main sequence star approximately 521 light-years away in the constellation of Lyra (the Lyre). [2][3] It hosts one …
We detected the transit light-curve signature in the course of the TrES multisite transiting planet survey and confirmed the planetary nature of the companion via multicolor photometry and …
TrES-1 | NASA Exoplanet Archive
Planetary transit observations at the University Observatory Jena: XO-1b and TrES-1 Raetz et al. 2009 | Reference Overview Improved Parameters for Extrasolar Transiting Planets
TrES-1: The Transiting Planet of a Bright K0 V Star - NASA/ADS
We report the detection of a transiting Jupiter-sized planet orbiting a relatively bright (V=11.79) K0 V star. We detected the transit light-curve signature in the course of the TrES multisite …
TrES-1b - ExoClock
The target uncertainty has been defined as the 1/12 of the target's transit duration (in 2029). CAMPAIGN : Planet included in one of the current observing campaings. TTVs : Planet …
Title: TrES-1: The Transiting Planet of a Bright K0V Star - arXiv.org
Aug 23, 2004 · We detected the transit light-curve signature in the course of the TrES multi-site transiting planet survey, and confirmed the planetary nature of the companion via multicolor …
TrES-1
TrES-1 is an exoplanet orbiting the star TrES-1, located about 512.1 light-years (157.0 pc) away from Solar System. Its discovery was publicly announced on 2004. The host star TrES-1 has …
TrES-1: The Transiting Planet of a Bright K0 V Star - IOPscience
Sep 1, 2004 · We report the detection of a transiting Jupiter-sized planet orbiting a relatively bright (V = 11.79) K0 V star. We detected the transit light-curve signature in the course of the TrES …