Kepler-43
Sign in to saveKepler-43, formerly known as KOI-135, is a star in the northern constellation of Lyra. At 14th magnitude, it is too faint to be seen with the naked eye.
Astronomical data · SIMBAD
- Object type
- EB*
- Spectral type
- G0
- Distance
- 3,313 light-years
- Redshift
- z = -0.00012436030256024466
- Coordinates
- RA 285.2408° · Dec 46.6682°
View on SIMBAD →
via SIMBAD · CDS Strasbourg
Wikidata facts
- Instance of
- rotating variable star
- Constellation
- Lyra
- Distance from Earth
- 1035.9
- Diameter
- 2020000
- Radius
- 1.42
- Mass
- 1.32
- Variable-star type
- eclipsing binary star
Show 16 more facts
- catalog code
- SPOCS 3999
- effective temperature
- 6041
- parallax
- 0.9846
- radial velocity
- -39.8
- apparent magnitude
- 13.876887
- surface gravity
- 33000
- spectral class
- F9
- epoch
- J2000.0
- metallicity
- 0.35
- stellar rotational velocity
- 4.8
- luminosity
- 2.2081122
- right ascension component of proper motion
- -2.982
- declination component of proper motion
- 0.126
- right ascension
- 285.24084751675
- declination
- 46.66824052435
- age estimated by a dating method
- 2.8
via Wikidata · CC0
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Encyclopedic overview
2 sectionsContents
- Planetary system
- References
Kepler-43, formerly known as KOI-135, is a star in the northern constellation of Lyra. At 14th magnitude, it is too faint to be seen with the naked eye.
Kepler-43 has a very strong starspot activity.
Excerpted from Wikipedia’s “Kepler-43” article, available under the CC BY-SA 4.0 licence.