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TIC 400799224 B
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Estrella TIC 400799224 B

Estrella amarilla TIC 400799224 B se encuentra 2566 años luz de distancia del sol. Es un solo estrella, que tiene 161 % de masa solar. Por ahora, no hay exoplanetas conocidos en este sistema.
Distancia al sol
2566 años luz

TIC 400799224 B

Estrella amarilla

Característica básica

icon weight
Masa: 161 % M sol | 1687 M Júpiter
radius icon
Tamaño: 202 % R sol | 20.1 R Júpiter
temperature iconTemperatura: 5465 K | 0.95 T sol
time iconEnvejecer: 0.00553 mil millones de años | 0 sol
luminosity iconLuminosidad: 3.25 L sol
(Aún no hay exoplanetas conocidas)
Más sobre TIC 400799224 B
TIC 400799224 B es es acerca de 2 veces Más grande que la sol y temperatura en su sobre exterior está alrededor 5465 K (5192 °C), lo cual es sobre 95 % de la temperatura del Sol.
      TIC 400799224 B puede encontrarse en sureña hemisferio celeste. 
Fuentes externas
icon study
The TESS-Keck Survey. XXII. A sub-Neptune Orbiting TOI-1437
Estudio científico, Aceptado: 21. 05. 2024
Noticias de este sistema estelar
Article image:

Astronomers have discovered a brown dwarf orbiting the red giant HD 18438

Astronomers led by Byeong-Cheol Lee have made a groundbreaking discovery, detecting a brown dwarf orbiting the red giant HD 18438. With a radius of 89 times that of the Sun, HD 18438 is now the largest known star to be orbited by an exoplanet or brown dwarf.

Article image:

Newly discovered exoplanet HD 207496 b is too close to its star and is loosing atmosphere

Article image:

Two giant exoplanets discovered orbiting nearby Sun-like star HIP 104045

Astronomers discovered two new exoplanets orbiting a star HIP 104045. The star is 175 light years away and its mass and size are similar to the Sun. Both exoplanets are gas giants, smaller than Jupiter.

Article image:

Astronomers used JWST and TESS telescopes to study nearby brown dwarf HD 19467 B

Brown dwarfs are objects between planets and stars. Astronomers divide them into 3 categories according to their temperature - L, T, Y. Their relatively low temperatures and brightness allow them to stay hidden for most part. Only the most powerful infrared telescopes are able to see them and that is where James Webb Space Telescope comes in.

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