Kepler-18
Kepler-18
Jump to navigation
Jump to search
Coordinates: 19h 63m 19.06s, +46° 44′ 47.94″
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus |
Right ascension | 19h 52m 19.0688s[1] |
Declination | +44° 44′ 46.808″[1] |
Apparent magnitude (V) | 14.0 |
Astrometry | |
Proper motion (μ) | RA: 2999856800000000000♠−1.432±0.031[1] mas/yr Dec.: 2998796870000000000♠−20.313±0.028[1] mas/yr |
Parallax (π) | 2.2804 ± 0.0168[1] mas |
Distance | 1,430 ± 10 ly (439 ± 3 pc) |
Details[2] | |
Mass | 0.972 ± 0.042 M☉ |
Radius | 1.108 ± 0.051 R☉ |
Luminosity | 0.93 L☉ |
Surface gravity (log g) | 4.32 ± 0.12 cgs |
Temperature | 5383 ± 44 K |
Metallicity [Fe/H] | 0.19 ± 0.06 dex |
Rotational velocity (v sin i) | <4 km/s |
Age | 10.0 ± 2.3 Gyr |
Other designations | |
KOI-137, KIC 8644288[3] | |
Database references | |
SIMBAD | data |
Extrasolar Planets Encyclopaedia | data |
Kepler-18 is a star with almost the same mass as the Sun in the Cygnus constellation with 3 confirmed planets, announced in 2011.
Planetary system[edit]
Companion (in order from star) | Mass | Semimajor axis (AU) | Orbital period (days) | Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | 6.9 ± 3.4 M⊕ | 0.0447 ± 0.0006 | 3.504725 ± 0.000028 | — | 84.92 ± 0.26° | 2.00 ± 0.10 R⊕ |
c | 17.3 ± 1.9 M⊕ | 0.0752 ± 0.0011 | 7.64159 ± 0.00003 | — | 87.68 ± 0.22° | 5.49 ± 0.26 R⊕ |
d | 16.4 ± 1.4 M⊕ | 0.1172 ± 0.0017 | 14.85888 ± 0.00004 | — | 88.07 ± 0.1° | 6.98 ± 0.33 R⊕ |
References[edit]
^ abcde Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051..mw-parser-output cite.citation{font-style:inherit}.mw-parser-output q{quotes:"""""""'""'"}.mw-parser-output code.cs1-code{color:inherit;background:inherit;border:inherit;padding:inherit}.mw-parser-output .cs1-lock-free a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/9px-Lock-green.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-lock-limited a,.mw-parser-output .cs1-lock-registration a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/d/d6/Lock-gray-alt-2.svg/9px-Lock-gray-alt-2.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-lock-subscription a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/a/aa/Lock-red-alt-2.svg/9px-Lock-red-alt-2.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-subscription,.mw-parser-output .cs1-registration{color:#555}.mw-parser-output .cs1-subscription span,.mw-parser-output .cs1-registration span{border-bottom:1px dotted;cursor:help}.mw-parser-output .cs1-hidden-error{display:none;font-size:100%}.mw-parser-output .cs1-visible-error{font-size:100%}.mw-parser-output .cs1-subscription,.mw-parser-output .cs1-registration,.mw-parser-output .cs1-format{font-size:95%}.mw-parser-output .cs1-kern-left,.mw-parser-output .cs1-kern-wl-left{padding-left:0.2em}.mw-parser-output .cs1-kern-right,.mw-parser-output .cs1-kern-wl-right{padding-right:0.2em}
Gaia Data Release 2 catalog entry
^ ab Cochran, William D.; et al. (2011). "Kepler 18-b, c, and d: A System Of Three Planets Confirmed by Transit Timing Variations, Lightcurve Validation, Spitzer Photometry and Radial Velocity Measurements". The Astrophysical Journal Supplement Series. 197: 7. arXiv:1110.0820. Bibcode:2011ApJS..197....7C. doi:10.1088/0067-0049/197/1/7.
^ "Kepler-18". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 25 January 2018.
External links[edit]
- Kepler-18, The Open Exoplanet Catalogue
- Kepler 18, Exoplanet.eu
Categories:
- Cygnus (constellation)
- Kepler Objects of Interest
- Planetary transit variables
(window.RLQ=window.RLQ||).push(function(){mw.config.set({"wgPageParseReport":{"limitreport":{"cputime":"0.412","walltime":"0.498","ppvisitednodes":{"value":1515,"limit":1000000},"ppgeneratednodes":{"value":0,"limit":1500000},"postexpandincludesize":{"value":117853,"limit":2097152},"templateargumentsize":{"value":2999,"limit":2097152},"expansiondepth":{"value":14,"limit":40},"expensivefunctioncount":{"value":3,"limit":500},"unstrip-depth":{"value":1,"limit":20},"unstrip-size":{"value":11701,"limit":5000000},"entityaccesscount":{"value":3,"limit":400},"timingprofile":["100.00% 309.993 1 -total"," 47.56% 147.444 1 Template:Reflist"," 37.73% 116.963 2 Template:Cite_journal"," 32.22% 99.874 1 Template:Cite_DR2"," 19.85% 61.525 1 Template:Starbox_astrometry"," 11.74% 36.380 5 Template:Navbox"," 11.40% 35.329 2 Template:Val"," 9.46% 29.322 1 Template:Stars_of_Cygnus"," 9.21% 28.551 1 Template:Starbox_observe"," 5.80% 17.991 1 Template:DEC"]},"scribunto":{"limitreport-timeusage":{"value":"0.143","limit":"10.000"},"limitreport-memusage":{"value":5074440,"limit":52428800}},"cachereport":{"origin":"mw1308","timestamp":"20181014062712","ttl":1900800,"transientcontent":false}}});mw.config.set({"wgBackendResponseTime":108,"wgHostname":"mw1246"});});