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ケプラー40
Sign in to saveKepler-40, formerly known as KOI-428, is an F-type star in the constellation Cygnus. Kepler-40 is known to host at least one planet, Kepler-40b. The star is approximately 1.5 times more massive than the Sun, and is over two times its size; it was, at upon its discovery, the largest yet discovered with a transiting planet in its orbit. Kepler-40 was first noted as home to a possible transiting object by the Kepler spacecraft; the data on the system was released to the public. A team of French and Swiss scientists used follow-up data to determine the existence of the Hot Jupiter planet Kepler-40
Astronomical data · SIMBAD
- Object type
- *
- Spectral type
- F5IV
- Distance
- 7,168 light-years
- Coordinates
- RA 296.8137° · Dec 47.5266°
via SIMBAD · CDS Strasbourg
Wikidata facts
- Constellation
- Cygnus
- Child body
- Kepler-40 b
- Distance from Earth
- 2700
- Radius
- 2.13
- Mass
- 1.48
- Variable-star type
- rotating variable star
Show 14 more facts
- surface gravity
- 35500
- catalog code
- TIC 272840455
- effective temperature
- 6510
- parallax
- 0.455
- apparent magnitude
- 14.547202
- metallicity
- 0.10
- epoch
- J2000.0
- spectral class
- F5 IV
- luminosity
- 6.77782
- right ascension component of proper motion
- -1.469
- declination component of proper motion
- -6.768
- right ascension
- 296.81369762414
- declination
- 47.52657370076
- age estimated by a dating method
- 2.8
via Wikidata · CC0
Article · 日本語
ケプラー40 (英: Kepler-40、KOI-428) とは、はくちょう座の方向に約8100光年離れた場所に位置する恒星である。ケプラー40は、少なくとも1つの惑星ケプラー40bを持っていることが知られている。この惑星の有無を判断するためにフォローアップ観測のデータの解析が行われ、その結果は2011年1月4日に科学雑誌に発表された。ケプラー40は太陽の約1.5倍の質量を持ち、そのサイズは2倍以上である。
Abstract from DBpedia / Wikipedia · CC BY-SA