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HD 190412 B
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Estrella HD 190412 B

Estrella naranja HD 190412 B se encuentra 111 años luz de distancia del sol. Es un solo estrella, que tiene 61 % de masa solar. Por ahora, no hay exoplanetas conocidos en este sistema.
Distancia al sol
111 años luz

HD 190412 B

Estrella naranja

Característica básica

icon weight
Masa: 61 % M sol | 639 M Júpiter
temperature iconTemperatura: 4130 K | 0.71 T sol
(Aún no hay exoplanetas conocidas)
Más sobre HD 190412 B
y temperatura en su sobre exterior está alrededor 4130 K (3857 °C), lo cual es sobre 71 % de la temperatura del Sol.
      HD 190412 B puede encontrarse en norteña hemisferio celeste. 
Fuentes externas
icon study
Into the red: an M-band study of the chemistry and rotation of
Estudio científico, Aceptado: 14. 05. 2024
icon study
TOI-2447 b / NGTS-29 b: a 69-day Saturn around a Solar analogue
Estudio científico, Aceptado: 12. 05. 2024
icon study
A secondary atmosphere on the rocky exoplanet 55 Cancri e
Estudio científico, Aceptado: 08. 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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