In this article, we will explore the fascinating history of TOI-1452 b, a topic that has captured the attention of millions of people around the world. From its origins to its impact on today's society, TOI-1452 b has left an indelible mark on different aspects of daily life. Over the next few pages, we will immerse ourselves in a journey through time to fully understand the importance of TOI-1452 b and its influence in various areas. From his contributions in _var2 to the innovations he has pioneered in _var3, TOI-1452 b has played a crucial role in shaping the world as we know it today. Join us on this exploration as we discover more about TOI-1452 b's shocking story.
Discovery | |
---|---|
Discovered by | Cadieux, Charles et al.; International Team |
Discovery site | Université de Montréal |
Discovery date | June 2022 |
Orbital characteristics | |
0.061±0.003 AU | |
Eccentricity | 0 |
11 days | |
Inclination | 89.77°±0.16° |
90 | |
Star | TOI-1452 |
Physical characteristics | |
Mean radius | 1.67±0.07 R🜨 |
Mass | 4.82±1.3 ME |
Mean density | 5.6+1.8 −1.6 g/cm3 |
Temperature | 326±7 K |
TOI-1452 b is a confirmed super-Earth exoplanet, possibly a water world, orbiting a red-dwarf star TOI-1452 about 100 light-years away in the Draco constellation. The exoplanet is about 70% larger in diameter than Earth, and roughly five times as massive.
The TOI-1452 star system is 99 light-years away from Earth, located in the constellation of Draco. It is a binary pair of dim red dwarf stars separated by only 96 astronomical units (AU). A notable feature of this system is the presence of an exoplanet around one of the stars, designated as TOI-1452 b. It is two M4 dwarf stars that were observed by TESS as a priority, since they are on the cool dwarf list, a list of high-priority orange-red and red dwarf stars, that was uploaded to TESS. It is a flare star, with a flare observed by TESS where the star brightened by 5%. The secondary star is often distinguished from the first with the name "TOI-1760".
TOI-1452 b was discovered by an international team led by astronomers from the Université de Montréal, using data from NASA’s Transiting Exoplanet Survey Satellite (TESS). The discovery was first reported in June 2022.
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