Kepler-14b: A massive hot Jupiter transiting an F star in a close visual binary

Lars A. Buchhave; David W. Latham; Joshua A. Carter; Jean Michel Désert; Guillermo Torres; Elisabeth R. Adams; Stephen T. Bryson; David B. Charbonneau; David R. Ciardi; Craig Kulesa; Andrea K. Dupree; Debra A. Fischer; François Fressin; Thomas N. Gautier; Ronald L. Gilliland; Steve B. Howell; Howard Isaacson; Jon M. Jenkins; Geoffrey W. Marcy; Donald W. McCarthy; Jason F. Rowe; Natalie M. Batalha; William J. Borucki; Timothy M. Brown; Douglas A. Caldwell; Jessie L. Christiansen; William D. Cochran; Drake Deming; Edward W. Dunham; Mark Everett; Eric B. Ford; Jonathan J. Fortney; John C. Geary; Forrest R. Girouard; Michael R. Haas; Matthew J. Holman; Elliott Horch; Todd C. Klaus; Heather A. Knutson; David G. Koch; Jeffrey Kolodziejczak; Jack J. Lissauer; Pavel MacHalek; Fergal Mullally; Martin D. Still; Samuel N. Quinn; Sara Seager; Susan E. Thompson; Jeffrey Van Cleve

doi:10.1088/0067-0049/197/1/3

Kepler-14b: A massive hot Jupiter transiting an F star in a close visual binary

Lars A. Buchhave, David W. Latham, Joshua A. Carter, Jean Michel Désert, Guillermo Torres, Elisabeth R. Adams, Stephen T. Bryson, David B. Charbonneau, David R. Ciardi, Craig Kulesa, Andrea K. Dupree, Debra A. Fischer, François Fressin, Thomas N. Gautier, Ronald L. Gilliland, Steve B. Howell, Howard Isaacson, Jon M. Jenkins, Geoffrey W. Marcy, Donald W. McCarthyJason F. Rowe, Natalie M. Batalha, William J. Borucki, Timothy M. Brown, Douglas A. Caldwell, Jessie L. Christiansen, William D. Cochran, Drake Deming, Edward W. Dunham, Mark Everett, Eric B. Ford, Jonathan J. Fortney, John C. Geary, Forrest R. Girouard, Michael R. Haas, Matthew J. Holman, Elliott Horch, Todd C. Klaus, Heather A. Knutson, David G. Koch, Jeffrey Kolodziejczak, Jack J. Lissauer, Pavel MacHalek, Fergal Mullally, Martin D. Still, Samuel N. Quinn, Sara Seager, Susan E. Thompson, Jeffrey Van Cleve

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Abstract

We present the discovery of a hot Jupiter transiting an F star in a close visual (03 sky projected angular separation) binary system. The dilution of the host star's light by the nearly equalmagnitude stellar companion (∼0.5mag fainter) significantly affects the derived planetary parameters, and if left uncorrected, leads to an underestimate of the radius and mass of the planet by 10% and 60%, respectively. Other published exoplanets, which have not been observed with high-resolution imaging, could similarly have unresolved stellar companions and thus have incorrectly derived planetary parameters. Kepler-14b (KOI-98) has a period of P = 6.790 days and, correcting for the dilution, has a mass of M_p = 8.40^+0.35 _-0.34 M _J and a radius of R_p = 1.136^+0.073_-0.054 R _J, yielding a mean density of ρ_p = 7.1 ± 1.1 g cm^-3.

Original language	English (US)
Article number	3
Journal	Astrophysical Journal, Supplement Series
Volume	197
Issue number	1
DOIs	https://doi.org/10.1088/0067-0049/197/1/3
State	Published - Nov 2011

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

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10.1088/0067-0049/197/1/3

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Buchhave, L. A., Latham, D. W., Carter, J. A., Désert, J. M., Torres, G., Adams, E. R., Bryson, S. T., Charbonneau, D. B., Ciardi, D. R., Kulesa, C., Dupree, A. K., Fischer, D. A., Fressin, F., Gautier, T. N., Gilliland, R. L., Howell, S. B., Isaacson, H., Jenkins, J. M., Marcy, G. W., ... Van Cleve, J. (2011). Kepler-14b: A massive hot Jupiter transiting an F star in a close visual binary. Astrophysical Journal, Supplement Series, 197(1), Article 3. https://doi.org/10.1088/0067-0049/197/1/3

@article{b40ed0753df2425a88715e796e300dc4,

title = "Kepler-14b: A massive hot Jupiter transiting an F star in a close visual binary",

abstract = "We present the discovery of a hot Jupiter transiting an F star in a close visual (03 sky projected angular separation) binary system. The dilution of the host star's light by the nearly equalmagnitude stellar companion (∼0.5mag fainter) significantly affects the derived planetary parameters, and if left uncorrected, leads to an underestimate of the radius and mass of the planet by 10% and 60%, respectively. Other published exoplanets, which have not been observed with high-resolution imaging, could similarly have unresolved stellar companions and thus have incorrectly derived planetary parameters. Kepler-14b (KOI-98) has a period of P = 6.790 days and, correcting for the dilution, has a mass of Mp = 8.40+0.35 -0.34 M J and a radius of Rp = 1.136+0.073-0.054 R J, yielding a mean density of ρp = 7.1 ± 1.1 g cm-3.",

author = "Buchhave, {Lars A.} and Latham, {David W.} and Carter, {Joshua A.} and D{\'e}sert, {Jean Michel} and Guillermo Torres and Adams, {Elisabeth R.} and Bryson, {Stephen T.} and Charbonneau, {David B.} and Ciardi, {David R.} and Craig Kulesa and Dupree, {Andrea K.} and Fischer, {Debra A.} and Fran{\c c}ois Fressin and Gautier, {Thomas N.} and Gilliland, {Ronald L.} and Howell, {Steve B.} and Howard Isaacson and Jenkins, {Jon M.} and Marcy, {Geoffrey W.} and McCarthy, {Donald W.} and Rowe, {Jason F.} and Batalha, {Natalie M.} and Borucki, {William J.} and Brown, {Timothy M.} and Caldwell, {Douglas A.} and Christiansen, {Jessie L.} and Cochran, {William D.} and Drake Deming and Dunham, {Edward W.} and Mark Everett and Ford, {Eric B.} and Fortney, {Jonathan J.} and Geary, {John C.} and Girouard, {Forrest R.} and Haas, {Michael R.} and Holman, {Matthew J.} and Elliott Horch and Klaus, {Todd C.} and Knutson, {Heather A.} and Koch, {David G.} and Jeffrey Kolodziejczak and Lissauer, {Jack J.} and Pavel MacHalek and Fergal Mullally and Still, {Martin D.} and Quinn, {Samuel N.} and Sara Seager and Thompson, {Susan E.} and {Van Cleve}, Jeffrey",

year = "2011",

month = nov,

doi = "10.1088/0067-0049/197/1/3",

language = "English (US)",

volume = "197",

journal = "Astrophysical Journal, Supplement Series",

issn = "0067-0049",

publisher = "American Astronomical Society",

number = "1",

}

Buchhave, LA, Latham, DW, Carter, JA, Désert, JM, Torres, G, Adams, ER, Bryson, ST, Charbonneau, DB, Ciardi, DR, Kulesa, C, Dupree, AK, Fischer, DA, Fressin, F, Gautier, TN, Gilliland, RL, Howell, SB, Isaacson, H, Jenkins, JM, Marcy, GW, McCarthy, DW, Rowe, JF, Batalha, NM, Borucki, WJ, Brown, TM, Caldwell, DA, Christiansen, JL, Cochran, WD, Deming, D, Dunham, EW, Everett, M, Ford, EB, Fortney, JJ, Geary, JC, Girouard, FR, Haas, MR, Holman, MJ, Horch, E, Klaus, TC, Knutson, HA, Koch, DG, Kolodziejczak, J, Lissauer, JJ, MacHalek, P, Mullally, F, Still, MD, Quinn, SN, Seager, S, Thompson, SE & Van Cleve, J 2011, 'Kepler-14b: A massive hot Jupiter transiting an F star in a close visual binary', Astrophysical Journal, Supplement Series, vol. 197, no. 1, 3. https://doi.org/10.1088/0067-0049/197/1/3

TY - JOUR

T1 - Kepler-14b

T2 - A massive hot Jupiter transiting an F star in a close visual binary

AU - Buchhave, Lars A.

AU - Latham, David W.

AU - Carter, Joshua A.

AU - Désert, Jean Michel

AU - Torres, Guillermo

AU - Adams, Elisabeth R.

AU - Bryson, Stephen T.

AU - Charbonneau, David B.

AU - Ciardi, David R.

AU - Kulesa, Craig

AU - Dupree, Andrea K.

AU - Fischer, Debra A.

AU - Fressin, François

AU - Gautier, Thomas N.

AU - Gilliland, Ronald L.

AU - Howell, Steve B.

AU - Isaacson, Howard

AU - Jenkins, Jon M.

AU - Marcy, Geoffrey W.

AU - McCarthy, Donald W.

AU - Rowe, Jason F.

AU - Batalha, Natalie M.

AU - Borucki, William J.

AU - Brown, Timothy M.

AU - Caldwell, Douglas A.

AU - Christiansen, Jessie L.

AU - Cochran, William D.

AU - Deming, Drake

AU - Dunham, Edward W.

AU - Everett, Mark

AU - Ford, Eric B.

AU - Fortney, Jonathan J.

AU - Geary, John C.

AU - Girouard, Forrest R.

AU - Haas, Michael R.

AU - Holman, Matthew J.

AU - Horch, Elliott

AU - Klaus, Todd C.

AU - Knutson, Heather A.

AU - Koch, David G.

AU - Kolodziejczak, Jeffrey

AU - Lissauer, Jack J.

AU - MacHalek, Pavel

AU - Mullally, Fergal

AU - Still, Martin D.

AU - Quinn, Samuel N.

AU - Seager, Sara

AU - Thompson, Susan E.

AU - Van Cleve, Jeffrey

PY - 2011/11

Y1 - 2011/11

N2 - We present the discovery of a hot Jupiter transiting an F star in a close visual (03 sky projected angular separation) binary system. The dilution of the host star's light by the nearly equalmagnitude stellar companion (∼0.5mag fainter) significantly affects the derived planetary parameters, and if left uncorrected, leads to an underestimate of the radius and mass of the planet by 10% and 60%, respectively. Other published exoplanets, which have not been observed with high-resolution imaging, could similarly have unresolved stellar companions and thus have incorrectly derived planetary parameters. Kepler-14b (KOI-98) has a period of P = 6.790 days and, correcting for the dilution, has a mass of Mp = 8.40+0.35 -0.34 M J and a radius of Rp = 1.136+0.073-0.054 R J, yielding a mean density of ρp = 7.1 ± 1.1 g cm-3.

AB - We present the discovery of a hot Jupiter transiting an F star in a close visual (03 sky projected angular separation) binary system. The dilution of the host star's light by the nearly equalmagnitude stellar companion (∼0.5mag fainter) significantly affects the derived planetary parameters, and if left uncorrected, leads to an underestimate of the radius and mass of the planet by 10% and 60%, respectively. Other published exoplanets, which have not been observed with high-resolution imaging, could similarly have unresolved stellar companions and thus have incorrectly derived planetary parameters. Kepler-14b (KOI-98) has a period of P = 6.790 days and, correcting for the dilution, has a mass of Mp = 8.40+0.35 -0.34 M J and a radius of Rp = 1.136+0.073-0.054 R J, yielding a mean density of ρp = 7.1 ± 1.1 g cm-3.

UR - http://www.scopus.com/inward/record.url?scp=80655127955&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=80655127955&partnerID=8YFLogxK

U2 - 10.1088/0067-0049/197/1/3

DO - 10.1088/0067-0049/197/1/3

M3 - Article

AN - SCOPUS:80655127955

SN - 0067-0049

VL - 197

JO - Astrophysical Journal, Supplement Series

JF - Astrophysical Journal, Supplement Series

IS - 1

M1 - 3

ER -

Kepler-14b: A massive hot Jupiter transiting an F star in a close visual binary

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