Kepler-17
Kepler-17
Jump to navigation
Jump to search
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus |
Right ascension | 19h 53m 34.8643s[1] |
Declination | +47° 48′ 54.050″[1] |
Apparent magnitude (V) | 14.0[2] |
Astrometry | |
Proper motion (μ) | RA: 2999622200000000000♠−3.778±0.032[1] mas/yr Dec.: 2999363500000000000♠−6.365±0.035[1] mas/yr |
Parallax (π) | 1.3589 ± 0.0198[1] mas |
Distance | 2,400 ± 30 ly (740 ± 10 pc) |
Characteristics | |
Spectral type | G2V[2] |
Details[2] | |
Mass | 7000115999999999999♠1.16±0.06 M☉ |
Radius | 7000105000000000000♠1.05±0.03 R☉ |
Temperature | 7003578100000000000♠5781±85 K |
Metallicity [Fe/H] | 0.26 (± 0.1) dex |
Rotation | 7001121590000000000♠12.159±0.029 days[3] |
Rotational velocity (v sin i) | 7000420000000000000♠4.2±0.5[4] km/s |
Age | <1.78 Gyr |
Other designations | |
KIC 10619192, KOI-203, 2MASS J19533486+4748540[4] | |
Database references | |
SIMBAD | data |
KIC | data |
Kepler-17 is a star around which the planet Kepler-17b orbits.
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
^ abc "Notes on Kepler-17 b". Retrieved 15 January 2017.
^ McQuillan, A.; Mazeh, T.; Aigrain, S. (2013). "Stellar Rotation Periods of The Kepler objects of Interest: A Dearth of Close-In Planets Around Fast Rotators". The Astrophysical Journal Letters. 775 (1). L11. arXiv:1308.1845. Bibcode:2013ApJ...775L..11M. doi:10.1088/2041-8205/775/1/L11.
^ ab "Kepler-17". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 16 January 2017.
- http://arxiv.org/pdf/1107.5750v1
- https://web.archive.org/web/20111113211334/http://exoplanet.eu/star.php?st=Kepler-17&showPubli=yes&sortByDate
Coordinates: 19h 53m 34.86s, +47° 48′ 54″
This extrasolar-planet-related article is a stub. You can help Wikipedia by expanding it. |
This main-sequence-star-related article is a stub. You can help Wikipedia by expanding it. |
Categories:
- Cygnus (constellation)
- G-type main-sequence stars
- Planetary transit variables
- Kepler Objects of Interest
- Exoplanet stubs
- Main-sequence-star stubs
(window.RLQ=window.RLQ||).push(function(){mw.config.set({"wgPageParseReport":{"limitreport":{"cputime":"0.384","walltime":"0.470","ppvisitednodes":{"value":1340,"limit":1000000},"ppgeneratednodes":{"value":0,"limit":1500000},"postexpandincludesize":{"value":123789,"limit":2097152},"templateargumentsize":{"value":4384,"limit":2097152},"expansiondepth":{"value":14,"limit":40},"expensivefunctioncount":{"value":3,"limit":500},"unstrip-depth":{"value":1,"limit":20},"unstrip-size":{"value":12961,"limit":5000000},"entityaccesscount":{"value":3,"limit":400},"timingprofile":["100.00% 306.670 1 -total"," 44.96% 137.892 1 Template:Reflist"," 34.05% 104.436 2 Template:Cite_journal"," 32.03% 98.212 1 Template:Cite_DR2"," 19.22% 58.940 1 Template:Starbox_astrometry"," 14.54% 44.595 7 Template:Val"," 9.50% 29.140 5 Template:Navbox"," 8.59% 26.346 1 Template:Starbox_observe"," 7.94% 24.359 1 Template:Stars_of_Cygnus"," 6.12% 18.769 1 Template:Starbox_detail"]},"scribunto":{"limitreport-timeusage":{"value":"0.140","limit":"10.000"},"limitreport-memusage":{"value":4708020,"limit":52428800}},"cachereport":{"origin":"mw1295","timestamp":"20181014062658","ttl":1900800,"transientcontent":false}}});mw.config.set({"wgBackendResponseTime":95,"wgHostname":"mw1246"});});