Misplaced Pages

Kepler-68b: Difference between revisions

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Browse history interactively← Previous editContent deleted Content addedVisualWikitext
Revision as of 16:32, 8 January 2014 editArtman40 (talk | contribs)2,039 edits Sourced changing← Previous edit Latest revision as of 00:17, 27 September 2023 edit undoCitation bot (talk | contribs)Bots5,445,342 edits Add: doi-access. | Use this bot. Report bugs. | Suggested by Whoop whoop pull up | #UCB_webform 441/1027 
(14 intermediate revisions by 9 users not shown)
Line 1: Line 1:
{{Infobox planet
{{Planetbox begin
| name=Kepler-68b | name = Kepler-68b
<!-- DISCOVERY -->
| discovery_ref = <ref name="Gilliland2013"/>
| discoverer = Gilliland ''et al.''
| discovery_site = ]
| discovered = 2013
| discovery_method = ], and ]s
<!-- DESIGNATIONS -->
| alt_names = {{odlist | KOI=246.01 }}<ref name="Simbad"/>
<!-- ORBITAL -->
| orbit_ref = <ref name="Mills2019"/><ref name="Gilliland2013"/>
| semimajor = {{val|0.06170|0.00056|ul=AU}}
| eccentricity =
| period = {{val|5.398763|u=days}}
| inclination = {{val|87.60|0.90|u=º}}
| semi-amplitude = {{val|2.7|0.48|0.46|ul=m/s}}
| star = ]
<!-- PHYS CHARS -->
| physical_ref = <ref name="Mills2019"/>
| mean_radius = {{val|2.31|0.06|0.09|ul=Earth radius}}
| mass = {{val|7.65|1.37|1.32|ul=Earth mass}}
<!-- ATMOSPHERE -->
<!-- NOTES -->
}} }}
{{Planetbox star
| star = ] (KOI 246)
| constell=
| RA = {{RA|19|24|07.76}}
| DEC= {{DEC|+49|02|25}}
| dist_pc = 135
| dist_ly = 440
| app_mag = 8.588
| mass = 1.079±0.051
| radius = 1.243±0.019
| temperature = 5793±74
| metallicity = 0.12±0.074
| age = 6.3 ± 1.7
}}
{{Planetbox character
| mass_earth = 5.79
| radius_earth = 2.31±0.07
| stellar_flux =
| density_cgs = 2.60±0.74
| temperature = 1280
}}
{{Planetbox orbit
| period = 5.398763
| semimajor = 0.06170
| eccentricity =
| inclination = 87.60±0.9
}}
{{Planetbox discovery
| discovery_date = 12 February 2013
| discoverers =
| discovery_method = ] (])
| detection_methods = Radial velocity
| discovery_status = Confirmed
}}
{{Planetbox catalog
| names = KOI 246.01
}}
{{Planetbox end}}


'''Kepler-68b''' is an ] orbiting the Sun-like star ] in the ]. Discovered by planetary-transit methods by the ] in February 2013, it has a radius of 2.31 ± 0.07 that of ] and a density of 2.46–4.3 g/cm<sup>3</sup>. It has an orbital period of 5.398763 days at a distance of about 0.0617 ] from its star.<ref name=Gilliland>{{cite web|last=Gilliland|first=Ronald L.|title=Kepler-68: Three Planets, One With a Density Between That of Earth and Ice Giants|url=http://arxiv.org/abs/1302.2596|publisher=Cornell University|accessdate=28 February 2013}}</ref> ] measurements were made to determine its mass to be 5.79 times that of Earth (0.026 ]). <ref>http://astro.berkeley.edu/~gmarcy/22kois.pdf</ref> '''Kepler-68b''' is an ] orbiting the Sun-like star ] in the ]. Discovered by planetary-transit methods by the ] in February 2013, it has a radius of 2.31 ± 0.07 that of ] and a density of 2.46–4.3 g/cm<sup>3</sup>. It has an orbital period of 5.398763 days at a distance of about 0.0617 ] from its star.<ref name="Gilliland2013"/> ] measurements were made to determine its mass to be 5.79 times that of Earth (0.026 ]).<ref name="Marcy2014"/>


With a density of 2.6 g/cm<sup>3</sup> it has physical characteristics of both a ] and a ].<ref> accessdate=8 January 2014}}</ref> With a density of 2.6 g/cm<sup>3</sup> it has physical characteristics of both a ] and a ].<ref name="Marcy2014"/>


==See also== ==See also==
Line 49: Line 33:


==References== ==References==
{{reflist}} {{reflist|refs=

<ref name="Gilliland2013">{{cite journal | title=Kepler-68: Three Planets, One with a Density Between That of Earth and Ice Giants | last1=Gilliland | first1=Ronald L. | last2=Marcy | first2=Geoffrey W. | last3=Rowe | first3=Jason F. | last4=Rogers | first4=Leslie | last5=Torres | first5=Guillermo | last6=Fressin | first6=Francois | last7=Lopez | first7=Eric D. | last8=Buchhave | first8=Lars A. | last9=Christensen-Dalsgaard | first9=Jørgen | last10=Désert | first10=Jean-Michel | last11=Henze | first11=Christopher E. | last12=Isaacson | first12=Howard | last13=Jenkins | first13=Jon M. | last14=Lissauer | first14=Jack J. | last15=Chaplin | first15=William J. | last16=Basu | first16=Sarbani | last17=Metcalfe | first17=Travis S. | last18=Elsworth | first18=Yvonne | last19=Handberg | first19=Rasmus | last20=Hekker | first20=Saskia | last21=Huber | first21=Daniel | last22=Karoff | first22=Christoffer | last23=Kjeldsen | first23=Hans | last24=Lund | first24=Mikkel N. | last25=Lundkvist | first25=Mia | last26=Miglio | first26=Andrea | last27=Charbonneau | first27=David | last28=Ford | first28=Eric B. | last29=Fortney | first29=Jonathan J. | last30=Haas | first30=Michael R. | display-authors=1 | journal=The Astrophysical Journal | volume=766 | issue=1 | at=40 | year=2013 | arxiv=1302.2596 | bibcode=2013ApJ...766...40G | bibcode-access=free | doi=10.1088/0004-637X/766/1/40 | doi-access=free }}</ref>

<ref name="Marcy2014">{{cite journal | title=Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets | last1=Marcy | first1=Geoffrey W. | last2=Isaacson | first2=Howard | last3=Howard | first3=Andrew W. | last4=Rowe | first4=Jason F. | last5=Jenkins | first5=Jon M. | last6=Bryson | first6=Stephen T. | last7=Latham | first7=David W. | last8=Howell | first8=Steve B. | last9=Gautier | first9=Thomas N. | last10=Batalha | first10=Natalie M. | last11=Rogers | first11=Leslie | last12=Ciardi | first12=David | last13=Fischer | first13=Debra A. | last14=Gilliland | first14=Ronald L. | last15=Kjeldsen | first15=Hans | last16=Christensen-Dalsgaard | first16=Jørgen | last17=Huber | first17=Daniel | last18=Chaplin | first18=William J. | last19=Basu | first19=Sarbani | last20=Buchhave | first20=Lars A. | last21=Quinn | first21=Samuel N. | last22=Borucki | first22=William J. | last23=Koch | first23=David G. | last24=Hunter | first24=Roger | last25=Caldwell | first25=Douglas A. | last26=Van Cleve | first26=Jeffrey | last27=Kolbl | first27=Rea | last28=Weiss | first28=Lauren M. | last29=Petigura | first29=Erik | last30=Seager | first30=Sara | display-authors=1 | journal=The Astrophysical Journal Supplement Series | volume=210 | issue=2 | at=20 | year=2014 | arxiv=1401.4195 | bibcode=2014ApJS..210...20M | bibcode-access=free | doi=10.1088/0067-0049/210/2/20 | doi-access=free }}</ref>

<ref name="Mills2019">{{cite journal | title=Long-period Giant Companions to Three Compact, Multiplanet Systems | last1=Mills | first1=Sean M. | last2=Howard | first2=Andrew W. | last3=Weiss | first3=Lauren M. | last4=Steffen | first4=Jason H. | last5=Isaacson | first5=Howard | last6=Fulton | first6=Benjamin J. | last7=Petigura | first7=Erik A. | last8=Kosiarek | first8=Molly R. | last9=Hirsch | first9=Lea A. | last10=Boisvert | first10=John H. | display-authors=1 | journal=The Astronomical Journal | volume=157 | issue=4 | at=145 | year=2019 | arxiv=1903.07186 | bibcode=2019AJ....157..145M | doi=10.3847/1538-3881/ab0899 | s2cid=119197547 | doi-access=free }}</ref>


<ref name="Simbad">{{cite simbad | title=Kepler-68b | access-date=2019-10-30 }}</ref>


{{Exoplanets}} }}{{Kepler-68}}
{{Kepler-68}}
{{2013 in space}} {{2013 in space}}


] ]
] ]
] ]
] ]

Latest revision as of 00:17, 27 September 2023

Kepler-68b
Discovery
Discovered byGilliland et al.
Discovery siteKepler Space Observatory
Discovery date2013
Detection methodTransits, and transit-timing variations
Designations
Alternative namesKOI-246.01
Orbital characteristics
Semi-major axis0.06170±0.00056 AU
Orbital period (sidereal)5.398763 d
Inclination87.60±0.90 º
Semi-amplitude2.7+0.48
−0.46 m/s
StarKepler-68
Physical characteristics
Mean radius2.31+0.06
−0.09 R🜨
Mass7.65+1.37
−1.32 M🜨

Kepler-68b is an exoplanet orbiting the Sun-like star Kepler-68 in the constellation of Cygnus. Discovered by planetary-transit methods by the Kepler space telescope in February 2013, it has a radius of 2.31 ± 0.07 that of Earth and a density of 2.46–4.3 g/cm. It has an orbital period of 5.398763 days at a distance of about 0.0617 AU from its star. Doppler measurements were made to determine its mass to be 5.79 times that of Earth (0.026 MJ).

With a density of 2.6 g/cm it has physical characteristics of both a super-Earth and a mini-Neptune.

See also

References

  1. ^ 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.
  2. "Kepler-68b". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-10-30.
  3. ^ Mills, Sean M.; et al. (2019). "Long-period Giant Companions to Three Compact, Multiplanet Systems". The Astronomical Journal. 157 (4). 145. arXiv:1903.07186. Bibcode:2019AJ....157..145M. doi:10.3847/1538-3881/ab0899. S2CID 119197547.
  4. ^ Marcy, Geoffrey W.; et al. (2014). "Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets". The Astrophysical Journal Supplement Series. 210 (2). 20. arXiv:1401.4195. Bibcode:2014ApJS..210...20M. doi:10.1088/0067-0049/210/2/20.
Kepler-68 system
Stars
Planets
2013 in space
Space probe launches Space probes launched in 2013
Space probes
Space observatories
  • IRIS (solar observation; Jun 2013)
  • Hisaki (ultraviolet observation; Sep 2013)
  • Gaia (astrometric observation; Dec 2013)


Impact events
Selected NEOs
Exoplanets Exoplanets discovered in 2013
Discoveries
Novae
Comets Comets in 2013
Space exploration


Stub icon

This extrasolar-planet-related article is a stub. You can help Misplaced Pages by expanding it.

Categories: