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 composition to Jupiter.

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 discovery was announced in 2004.

TrES-1 0.85 R⦿ 5250.00 K TrES-1 b 1.130 RJup TrES-1 B Overview Notes System Parameters Ancillary Nearby Data Legend Expand All Architecture TrES-1 TrES-1 TrES-1 b TrES-1 B Other Data Bibliography 23 Exoplanet Archive Notes 1 TrES-1 …

TrES-1 is thus a graphic demonstration of the utility of a longitude-distributed network of transit-detection telescopes. The R-band transit seen by TrES has a flat-bottomed shape, a depth of 0.023 mag, and a total duration of about 3 hr.

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 known exoplanet, TrES-1b.

The Trans-Atlantic Exoplanet Survey, or TrES, used three 4-inch (10 cm) telescopes located at Lowell Observatory, Palomar Observatory, and Teide Observatory to locate exoplanets. It was made using the network of small, relatively inexpensive telescopes designed to look specifically for planets orbiting bright stars using the transit method.

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 composition to Jupiter.

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 photometry and precise radial velocity measurements.

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 transiting planet survey and confirmed the planetary nature of the companion via multicolor photometry and precise radial velocity measurements.

Exoplanet TrES-1 b orbits star TrES-1 that lies 521 light years away from the Sun. It weighs about 241.9 Earth masses and orbits its star much closer than Earth orbits Sun.