Kepler-16: A transiting circumbinary planet

Laurance R. Doyle; Joshua A. Carter; Daniel C. Fabrycky; Robert W. Slawson; Steve B. Howell; Joshua N. Winn; Jerome A. Orosz; Andrej Přsa; William F. Welsh; Samuel N. Quinn; David Latham; Guillermo Torres; Lars A. Buchhave; Geoffrey W. Marcy; Jonathan J. Fortney; Avi Shporer; Eric B. Ford; Jack J. Lissauer; Darin Ragozzine; Michael Rucker; Natalie Batalha; Jon M. Jenkins; William J. Borucki; David Koch; Christopher K. Middour; Jennifer R. Hall; Sean McCauliff; Michael N. Fanelli; Elisa V. Quintana; Matthew J. Holman; Douglas A. Caldwell; Martin Still; Robert P. Stefanik; Warren R. Brown; Gilbert A. Esquerdo; Sumin Tang; Gabor Furesz; John C. Geary; Perry Berlind; Michael L. Calkins; Donald R. Short; Jason H. Steffen; Dimitar Sasselov; Edward W. Dunham; William D. Cochran; Alan Boss; Michael R. Haas; Derek Buzasi; Debra Fischer

doi:10.1126/science.1210923

Kepler-16: A transiting circumbinary planet

Laurance R. Doyle, Joshua A. Carter, Daniel C. Fabrycky, Robert W. Slawson, Steve B. Howell, Joshua N. Winn, Jerome A. Orosz, Andrej Přsa, William F. Welsh, Samuel N. Quinn, David Latham, Guillermo Torres, Lars A. Buchhave, Geoffrey W. Marcy, Jonathan J. Fortney, Avi Shporer, Eric B. Ford, Jack J. Lissauer, Darin Ragozzine, Michael RuckerNatalie Batalha, Jon M. Jenkins, William J. Borucki, David Koch, Christopher K. Middour, Jennifer R. Hall, Sean McCauliff, Michael N. Fanelli, Elisa V. Quintana, Matthew J. Holman, Douglas A. Caldwell, Martin Still, Robert P. Stefanik, Warren R. Brown, Gilbert A. Esquerdo, Sumin Tang, Gabor Furesz, John C. Geary, Perry Berlind, Michael L. Calkins, Donald R. Short, Jason H. Steffen, Dimitar Sasselov, Edward W. Dunham, William D. Cochran, Alan Boss, Michael R. Haas, Derek Buzasi, Debra Fischer

Research output: Contribution to journal › Article › peer-review

554 Scopus citations

Abstract

We report the detection of a planet whose orbit surrounds a pair of low-mass stars. Data from the Kepler spacecraft reveal transits of the planet across both stars, in addition to the mutual eclipses of the stars, giving precise constraints on the absolute dimensions of all three bodies. The planet is comparable to Saturn in mass and size and is on a nearly circular 229-day orbit around its two parent stars. The eclipsing stars are 20 and 69% as massive as the Sun and have an eccentric 41-day orbit. The motions of all three bodies are confined to within 0.5° of a single plane, suggesting that the planet formed within a circumbinary disk.

Original language	English (US)
Pages (from-to)	1602-1606
Number of pages	5
Journal	Science
Volume	333
Issue number	6049
DOIs	https://doi.org/10.1126/science.1210923
State	Published - Sep 16 2011

All Science Journal Classification (ASJC) codes

General

Access to Document

10.1126/science.1210923

Cite this

Doyle, L. R., Carter, J. A., Fabrycky, D. C., Slawson, R. W., Howell, S. B., Winn, J. N., Orosz, J. A., Přsa, A., Welsh, W. F., Quinn, S. N., Latham, D., Torres, G., Buchhave, L. A., Marcy, G. W., Fortney, J. J., Shporer, A., Ford, E. B., Lissauer, J. J., Ragozzine, D., ... Fischer, D. (2011). Kepler-16: A transiting circumbinary planet. Science, 333(6049), 1602-1606. https://doi.org/10.1126/science.1210923

@article{041bbf5065144912a29832c8ead1b475,

title = "Kepler-16: A transiting circumbinary planet",

abstract = "We report the detection of a planet whose orbit surrounds a pair of low-mass stars. Data from the Kepler spacecraft reveal transits of the planet across both stars, in addition to the mutual eclipses of the stars, giving precise constraints on the absolute dimensions of all three bodies. The planet is comparable to Saturn in mass and size and is on a nearly circular 229-day orbit around its two parent stars. The eclipsing stars are 20 and 69% as massive as the Sun and have an eccentric 41-day orbit. The motions of all three bodies are confined to within 0.5° of a single plane, suggesting that the planet formed within a circumbinary disk.",

author = "Doyle, {Laurance R.} and Carter, {Joshua A.} and Fabrycky, {Daniel C.} and Slawson, {Robert W.} and Howell, {Steve B.} and Winn, {Joshua N.} and Orosz, {Jerome A.} and Andrej P{\v r}sa and Welsh, {William F.} and Quinn, {Samuel N.} and David Latham and Guillermo Torres and Buchhave, {Lars A.} and Marcy, {Geoffrey W.} and Fortney, {Jonathan J.} and Avi Shporer and Ford, {Eric B.} and Lissauer, {Jack J.} and Darin Ragozzine and Michael Rucker and Natalie Batalha and Jenkins, {Jon M.} and Borucki, {William J.} and David Koch and Middour, {Christopher K.} and Hall, {Jennifer R.} and Sean McCauliff and Fanelli, {Michael N.} and Quintana, {Elisa V.} and Holman, {Matthew J.} and Caldwell, {Douglas A.} and Martin Still and Stefanik, {Robert P.} and Brown, {Warren R.} and Esquerdo, {Gilbert A.} and Sumin Tang and Gabor Furesz and Geary, {John C.} and Perry Berlind and Calkins, {Michael L.} and Short, {Donald R.} and Steffen, {Jason H.} and Dimitar Sasselov and Dunham, {Edward W.} and Cochran, {William D.} and Alan Boss and Haas, {Michael R.} and Derek Buzasi and Debra Fischer",

year = "2011",

month = sep,

day = "16",

doi = "10.1126/science.1210923",

language = "English (US)",

volume = "333",

pages = "1602--1606",

journal = "Science",

issn = "0036-8075",

publisher = "American Association for the Advancement of Science",

number = "6049",

}

Doyle, LR, Carter, JA, Fabrycky, DC, Slawson, RW, Howell, SB, Winn, JN, Orosz, JA, Přsa, A, Welsh, WF, Quinn, SN, Latham, D, Torres, G, Buchhave, LA, Marcy, GW, Fortney, JJ, Shporer, A, Ford, EB, Lissauer, JJ, Ragozzine, D, Rucker, M, Batalha, N, Jenkins, JM, Borucki, WJ, Koch, D, Middour, CK, Hall, JR, McCauliff, S, Fanelli, MN, Quintana, EV, Holman, MJ, Caldwell, DA, Still, M, Stefanik, RP, Brown, WR, Esquerdo, GA, Tang, S, Furesz, G, Geary, JC, Berlind, P, Calkins, ML, Short, DR, Steffen, JH, Sasselov, D, Dunham, EW, Cochran, WD, Boss, A, Haas, MR, Buzasi, D & Fischer, D 2011, 'Kepler-16: A transiting circumbinary planet', Science, vol. 333, no. 6049, pp. 1602-1606. https://doi.org/10.1126/science.1210923

TY - JOUR

T1 - Kepler-16

T2 - A transiting circumbinary planet

AU - Doyle, Laurance R.

AU - Carter, Joshua A.

AU - Fabrycky, Daniel C.

AU - Slawson, Robert W.

AU - Howell, Steve B.

AU - Winn, Joshua N.

AU - Orosz, Jerome A.

AU - Přsa, Andrej

AU - Welsh, William F.

AU - Quinn, Samuel N.

AU - Latham, David

AU - Torres, Guillermo

AU - Buchhave, Lars A.

AU - Marcy, Geoffrey W.

AU - Fortney, Jonathan J.

AU - Shporer, Avi

AU - Ford, Eric B.

AU - Lissauer, Jack J.

AU - Ragozzine, Darin

AU - Rucker, Michael

AU - Batalha, Natalie

AU - Jenkins, Jon M.

AU - Borucki, William J.

AU - Koch, David

AU - Middour, Christopher K.

AU - Hall, Jennifer R.

AU - McCauliff, Sean

AU - Fanelli, Michael N.

AU - Quintana, Elisa V.

AU - Holman, Matthew J.

AU - Caldwell, Douglas A.

AU - Still, Martin

AU - Stefanik, Robert P.

AU - Brown, Warren R.

AU - Esquerdo, Gilbert A.

AU - Tang, Sumin

AU - Furesz, Gabor

AU - Geary, John C.

AU - Berlind, Perry

AU - Calkins, Michael L.

AU - Short, Donald R.

AU - Steffen, Jason H.

AU - Sasselov, Dimitar

AU - Dunham, Edward W.

AU - Cochran, William D.

AU - Boss, Alan

AU - Haas, Michael R.

AU - Buzasi, Derek

AU - Fischer, Debra

PY - 2011/9/16

Y1 - 2011/9/16

N2 - We report the detection of a planet whose orbit surrounds a pair of low-mass stars. Data from the Kepler spacecraft reveal transits of the planet across both stars, in addition to the mutual eclipses of the stars, giving precise constraints on the absolute dimensions of all three bodies. The planet is comparable to Saturn in mass and size and is on a nearly circular 229-day orbit around its two parent stars. The eclipsing stars are 20 and 69% as massive as the Sun and have an eccentric 41-day orbit. The motions of all three bodies are confined to within 0.5° of a single plane, suggesting that the planet formed within a circumbinary disk.

AB - We report the detection of a planet whose orbit surrounds a pair of low-mass stars. Data from the Kepler spacecraft reveal transits of the planet across both stars, in addition to the mutual eclipses of the stars, giving precise constraints on the absolute dimensions of all three bodies. The planet is comparable to Saturn in mass and size and is on a nearly circular 229-day orbit around its two parent stars. The eclipsing stars are 20 and 69% as massive as the Sun and have an eccentric 41-day orbit. The motions of all three bodies are confined to within 0.5° of a single plane, suggesting that the planet formed within a circumbinary disk.

UR - http://www.scopus.com/inward/record.url?scp=80052924665&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=80052924665&partnerID=8YFLogxK

U2 - 10.1126/science.1210923

DO - 10.1126/science.1210923

M3 - Article

C2 - 21921192

AN - SCOPUS:80052924665

SN - 0036-8075

VL - 333

SP - 1602

EP - 1606

JO - Science

JF - Science

IS - 6049

ER -

Kepler-16: A transiting circumbinary planet

Abstract

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this