| Discovery | |
|---|---|
| Discovery date | February 12, 2013 |
| Radial velocity | |
| Orbital characteristics | |
| Periastron | 1.148 AU |
| Apoastron | 1.652 AU |
| 1.4±0.03 AU [1] | |
| Eccentricity | 0.18 ± 0.05 |
| 580±50 d | |
| Physical characteristics | |
| Mass | ≥0.947 Mj |
Kepler-68d is a gas giant with the minimum mass about the same as Jupiter. It is at least a jovian-mass planet orbiting 1.4 astronomical units from its parent star, Kepler-68, well within habitable zone of the star. [2] It was detected by radial velocity. [3]
After planets Kepler-68b and c were detected by observing planetary transits in front of its star, doppler spectroscopy measurements were used to make follow-up observations of the star. Kepler-68d was discovered using that method.
References
- ^ "Kepler Discoveries". kepler.nasa.gov. Archived from the original on May 27, 2010. Retrieved February 26, 2013.
- ^ Gilliland, Ronald L.; et al. (2013). "Kepler-68: Three Planets, One with a Density Between That of Earth and Ice Giants". The Astrophysical Journal. 766 (1). 40. arXiv: 1302.2596. Bibcode: 2013ApJ...766...40G. doi: 10.1088/0004-637X/766/1/40. S2CID 7203273.
- ^ Exoplanet. "Planet Kepler-68 d". Exoplanet.eu. Archived from the original on 16 February 2014. Retrieved 28 February 2013.
External links
- Table of confirmed planets at NASA, Kepler mission
2013 in space | ||||||
|---|---|---|---|---|---|---|
Space probe launches
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|    | ||||
| Impact events | ||||||
| Selected NEOs | ||||||
|
Exoplanets
|
| |||||
| Discoveries |
| |||||
| Novae | ||||||
| Comets
| ||||||
| Space exploration |
| |||||
| Discovery | |
|---|---|
| Discovery date | February 12, 2013 |
| Radial velocity | |
| Orbital characteristics | |
| Periastron | 1.148 AU |
| Apoastron | 1.652 AU |
| 1.4±0.03 AU [1] | |
| Eccentricity | 0.18 ± 0.05 |
| 580±50 d | |
| Physical characteristics | |
| Mass | ≥0.947 Mj |
Kepler-68d is a gas giant with the minimum mass about the same as Jupiter. It is at least a jovian-mass planet orbiting 1.4 astronomical units from its parent star, Kepler-68, well within habitable zone of the star. [2] It was detected by radial velocity. [3]
After planets Kepler-68b and c were detected by observing planetary transits in front of its star, doppler spectroscopy measurements were used to make follow-up observations of the star. Kepler-68d was discovered using that method.
References
- ^ "Kepler Discoveries". kepler.nasa.gov. Archived from the original on May 27, 2010. Retrieved February 26, 2013.
- ^ Gilliland, Ronald L.; et al. (2013). "Kepler-68: Three Planets, One with a Density Between That of Earth and Ice Giants". The Astrophysical Journal. 766 (1). 40. arXiv: 1302.2596. Bibcode: 2013ApJ...766...40G. doi: 10.1088/0004-637X/766/1/40. S2CID 7203273.
- ^ Exoplanet. "Planet Kepler-68 d". Exoplanet.eu. Archived from the original on 16 February 2014. Retrieved 28 February 2013.
External links
- Table of confirmed planets at NASA, Kepler mission
2013 in space | ||||||
|---|---|---|---|---|---|---|
|
Space probe launches
|
| | ||||
| Impact events | ||||||
| Selected NEOs | ||||||
|
Exoplanets
|
| |||||
| Discoveries |
| |||||
| Novae | ||||||
| Comets
| ||||||
| Space exploration |
| |||||