HD 216770
ObjectStars
A late G-type dwarf star in Piscis Austrinus with an orbiting exoplanet.
1.00Common
Common
HD 216770
- Stars
HD 216770 is a late G-type main-sequence star, or yellow dwarf, in the southern constellation of Piscis Austrinus. It lies 120 light years from the Sun and is too faint to see with the naked eye. Smaller and less luminous than the Sun, it has high proper motion and an estimated age of about three billion years. An exoplanet announced in 2003 orbits the star every 118.5 days.
The picture on this card was made with AI. It is an illustration, not a real photo of the subject.
- Constellation
- Piscis Austrinus
- Distance from the Sun
- 120 light years
- Exoplanet orbital period
- 118.5 days
Sources and credits
Sources and credits
- Article
- HD 216770 (English Wikipedia)
- Wikidata
- Q1563281
- Text
- Card text is adapted from the English Wikipedia article by an automated summary. Wikipedia content is available under CC BY-SA 4.0; see the article history for its contributors. CC BY-SA 4.0 · Article history and contributors
- Illustration
- AI-generated illustration. Not a photograph or documentary image. (model: gpt-image-2.5-flare)
- Popularity
- 1 median daily views (Wikimedia Pageviews API (all-access, user agent))
Kosmora is not affiliated with or endorsed by the Wikimedia Foundation.