The planet of eternal night, TrES-2 b (named also TrES-2, TrES-2 A b, and Kepler-1 b) is an extrasolar planet orbiting the star GSC 03549-02811, located in the constellation Draco. On August 21, 2006, Trans-Atlantic Exoplanet Survey (TrES) discovered this exoplanet through the transit it made across its parent star using Sleuth (Palomar Observatory, California) and PSST (Lowell Observatory, Arizona). TrES-2 b was confirmed by the W.M.Keck Observatory on September 8, 2006, based on measurements of the star that hosts it.
In 2011, it was determined that TrES-2 b is the darkest exoplanet known so far, but today WASP-12b took its throne of being darker, reflecting less than 1% of all light that strikes it, thus it is named the "Dark world".
Using TrES-2 b's diameter of 181,880 km (113,014.992 miles), we are able to calculate its surface area, which is 103,924,935,529 km² (40,125,641,934.1314 miles²).
TrES-2 b has no surface such as Jupiter. Its interior structure is yet unknown.
We still do not know the density of TrES-2 b, but we do know its mass which is of 2,378,194,000,000,000,000,000,000 tons.
Studies of the tectonic plates of TrES-2 b has yet to be made.
The distance between TrES-2 b and its star is only 0.03227340053 AU (4,828,032 km or 3,000,000 miles).
TrES-2 b is situated 750.2 light years (7,097,440,000,000,000 km or 4,410,144,754,632,943.5 miles) away from Earth.
As indicated by its mass and radius, TrES-2 b is a gas giant with a bulk composition similar to that of Jupiter. The atmosphere of this exoplanet includes vaporized sodium, potassium, and titanium oxide, which actually add to the problem by absorbing heat. Still, TrES-2 b's extreme blackness is not fully explained.
TrES-2 b has a calculated temperature of 1455.0 K (1181.85°C or 2159.33°F).
The age of TrES-2 b is 5.1 billion years.
TrES-2 b has a gravitational force of 32.21 m/s² (105.675853 ft/s²).
It is still not known.
It takes 59 terrestrial hours (2.45833 Earth days) for TrES-2 b to make a full orbit aroud its host Star TrES-2.
It is thought that TrES-2 b is tidally locked like our moon, so one side of the planet is always facing the star, which means it has no days.
No moons have yet been found near TrES-2 b, but it is now being closely studied for signs of a possible satellite.
TrES-2 b has no ring.
Author: William Homier
Editor: William Homier
This page was last edited on 11 April 2022, at 19:50 (HAE).
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