Kepler-36: a pair of planets with neighboring orbits and dissimilar densities

Joshua A. Carter; Eric Agol; William J. Chaplin; Serbani Basu; Timothy R. Bedding; Lars A. Buchhave; Jørgen Christensen-Dalsgaard; Katherine M. Deck; Yvonne Elsworth; Daniel C. Fabrycky; Eric B. Ford; Jonathan J. Fortney; Steven J. Hale; Rasmus Handberg; Saskia Hekker; Matthew J. Holman; Daniel Huber; Christopher Karoff; Steven D. Kawaler; Hans Kjeldsen; Jack J. Lissauer; Eric D. Lopez; Mikkel N. Lund; Mia Lundkvist; Travis S. Metcalfe; Andrea Miglio; Leslie A. Rogers; Dennis Stello; William J. Borucki; Steve Bryson; Jessie L. Christiansen; William D. Cochran; John C. Geary; Ronald L. Gilliland; Michael R. Haas; Jennifer Hall; Andrew W. Howard; Jon M. Jenkins; Todd Klaus; David D. Koch; David W. Lathan; Phillip J. MacQueen; Dimitar Sasselov; Jason H. Steffen; Joseph D. Twicken; Joshua N. Winn

doi:10.1126/science.1223269

Kepler-36: a pair of planets with neighboring orbits and dissimilar densities

Joshua A. Carter, Eric Agol, William J. Chaplin, Serbani Basu, Timothy R. Bedding, Lars A. Buchhave, Jørgen Christensen-Dalsgaard, Katherine M. Deck, Yvonne Elsworth, Daniel C. Fabrycky, Eric B. Ford, Jonathan J. Fortney, Steven J. Hale, Rasmus Handberg, Saskia Hekker, Matthew J. Holman, Daniel Huber, Christopher Karoff, Steven D. Kawaler, Hans KjeldsenJack J. Lissauer, Eric D. Lopez, Mikkel N. Lund, Mia Lundkvist, Travis S. Metcalfe, Andrea Miglio, Leslie A. Rogers, Dennis Stello, William J. Borucki, Steve Bryson, Jessie L. Christiansen, William D. Cochran, John C. Geary, Ronald L. Gilliland, Michael R. Haas, Jennifer Hall, Andrew W. Howard, Jon M. Jenkins, Todd Klaus, David D. Koch, David W. Lathan, Phillip J. MacQueen, Dimitar Sasselov, Jason H. Steffen, Joseph D. Twicken, Joshua N. Winn

Astrofysik og Planetforskning

262 Citationer (Scopus)

Abstract

In the solar system, the planets' compositions vary with orbital distance, with rocky planets in close orbits and lower-density gas giants in wider orbits. The detection of close-in giant planets around other stars was the first clue that this pattern is not universal and that planets' orbits can change substantially after their formation. Here, we report another violation of the orbitcomposition pattern: two planets orbiting the same star with orbital distances differing by only 10% and densities differing by a factor of 8. One planet is likely a rocky "super-Earth," whereas the other is more akin to Neptune. These planets are 20 times more closely spaced and have a larger density contrast than any adjacent pair of planets in the solar system.

Originalsprog	Engelsk
Tidsskrift	Science
Vol/bind	337
Udgave nummer	6094
Sider (fra-til)	556-559
Antal sider	4
ISSN	0036-8075
DOI	https://doi.org/10.1126/science.1223269
Status	Udgivet - 3 aug. 2012

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10.1126/science.1223269

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Carter, J. A., Agol, E., Chaplin, W. J., Basu, S., Bedding, T. R., Buchhave, L. A., Christensen-Dalsgaard, J., Deck, K. M., Elsworth, Y., Fabrycky, D. C., Ford, E. B., Fortney, J. J., Hale, S. J., Handberg, R., Hekker, S., Holman, M. J., Huber, D., Karoff, C., Kawaler, S. D., ... Winn, J. N. (2012). Kepler-36: a pair of planets with neighboring orbits and dissimilar densities. Science, 337(6094), 556-559. https://doi.org/10.1126/science.1223269

Carter, JA, Agol, E, Chaplin, WJ, Basu, S, Bedding, TR, Buchhave, LA, Christensen-Dalsgaard, J, Deck, KM, Elsworth, Y, Fabrycky, DC, Ford, EB, Fortney, JJ, Hale, SJ, Handberg, R, Hekker, S, Holman, MJ, Huber, D, Karoff, C, Kawaler, SD, Kjeldsen, H, Lissauer, JJ, Lopez, ED, Lund, MN, Lundkvist, M, Metcalfe, TS, Miglio, A, Rogers, LA, Stello, D, Borucki, WJ, Bryson, S, Christiansen, JL, Cochran, WD, Geary, JC, Gilliland, RL, Haas, MR, Hall, J, Howard, AW, Jenkins, JM, Klaus, T, Koch, DD, Lathan, DW, MacQueen, PJ, Sasselov, D, Steffen, JH, Twicken, JD & Winn, JN 2012, 'Kepler-36: a pair of planets with neighboring orbits and dissimilar densities', Science, bind 337, nr. 6094, s. 556-559. https://doi.org/10.1126/science.1223269

@article{e2d8a50753e6404d9e4c61025a455e69,

title = "Kepler-36: a pair of planets with neighboring orbits and dissimilar densities",

abstract = "In the solar system, the planets' compositions vary with orbital distance, with rocky planets in close orbits and lower-density gas giants in wider orbits. The detection of close-in giant planets around other stars was the first clue that this pattern is not universal and that planets' orbits can change substantially after their formation. Here, we report another violation of the orbitcomposition pattern: two planets orbiting the same star with orbital distances differing by only 10% and densities differing by a factor of 8. One planet is likely a rocky {"}super-Earth,{"} whereas the other is more akin to Neptune. These planets are 20 times more closely spaced and have a larger density contrast than any adjacent pair of planets in the solar system.",

author = "Carter, {Joshua A.} and Eric Agol and Chaplin, {William J.} and Serbani Basu and Bedding, {Timothy R.} and Buchhave, {Lars A.} and J{\o}rgen Christensen-Dalsgaard and Deck, {Katherine M.} and Yvonne Elsworth and Fabrycky, {Daniel C.} and Ford, {Eric B.} and Fortney, {Jonathan J.} and Hale, {Steven J.} and Rasmus Handberg and Saskia Hekker and Holman, {Matthew J.} and Daniel Huber and Christopher Karoff and Kawaler, {Steven D.} and Hans Kjeldsen and Lissauer, {Jack J.} and Lopez, {Eric D.} and Lund, {Mikkel N.} and Mia Lundkvist and Metcalfe, {Travis S.} and Andrea Miglio and Rogers, {Leslie A.} and Dennis Stello and Borucki, {William J.} and Steve Bryson and Christiansen, {Jessie L.} and Cochran, {William D.} and Geary, {John C.} and Gilliland, {Ronald L.} and Haas, {Michael R.} and Jennifer Hall and Howard, {Andrew W.} and Jenkins, {Jon M.} and Todd Klaus and Koch, {David D.} and Lathan, {David W.} and MacQueen, {Phillip J.} and Dimitar Sasselov and Steffen, {Jason H.} and Twicken, {Joseph D.} and Winn, {Joshua N.}",

year = "2012",

month = aug,

day = "3",

doi = "10.1126/science.1223269",

language = "English",

volume = "337",

pages = "556--559",

journal = "Science",

issn = "0036-8075",

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

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TY - JOUR

T1 - Kepler-36

T2 - a pair of planets with neighboring orbits and dissimilar densities

AU - Carter, Joshua A.

AU - Agol, Eric

AU - Chaplin, William J.

AU - Basu, Serbani

AU - Bedding, Timothy R.

AU - Buchhave, Lars A.

AU - Christensen-Dalsgaard, Jørgen

AU - Deck, Katherine M.

AU - Elsworth, Yvonne

AU - Fabrycky, Daniel C.

AU - Ford, Eric B.

AU - Fortney, Jonathan J.

AU - Hale, Steven J.

AU - Handberg, Rasmus

AU - Hekker, Saskia

AU - Holman, Matthew J.

AU - Huber, Daniel

AU - Karoff, Christopher

AU - Kawaler, Steven D.

AU - Kjeldsen, Hans

AU - Lissauer, Jack J.

AU - Lopez, Eric D.

AU - Lund, Mikkel N.

AU - Lundkvist, Mia

AU - Metcalfe, Travis S.

AU - Miglio, Andrea

AU - Rogers, Leslie A.

AU - Stello, Dennis

AU - Borucki, William J.

AU - Bryson, Steve

AU - Christiansen, Jessie L.

AU - Cochran, William D.

AU - Geary, John C.

AU - Gilliland, Ronald L.

AU - Haas, Michael R.

AU - Hall, Jennifer

AU - Howard, Andrew W.

AU - Jenkins, Jon M.

AU - Klaus, Todd

AU - Koch, David D.

AU - Lathan, David W.

AU - MacQueen, Phillip J.

AU - Sasselov, Dimitar

AU - Steffen, Jason H.

AU - Twicken, Joseph D.

AU - Winn, Joshua N.

PY - 2012/8/3

Y1 - 2012/8/3

N2 - In the solar system, the planets' compositions vary with orbital distance, with rocky planets in close orbits and lower-density gas giants in wider orbits. The detection of close-in giant planets around other stars was the first clue that this pattern is not universal and that planets' orbits can change substantially after their formation. Here, we report another violation of the orbitcomposition pattern: two planets orbiting the same star with orbital distances differing by only 10% and densities differing by a factor of 8. One planet is likely a rocky "super-Earth," whereas the other is more akin to Neptune. These planets are 20 times more closely spaced and have a larger density contrast than any adjacent pair of planets in the solar system.

AB - In the solar system, the planets' compositions vary with orbital distance, with rocky planets in close orbits and lower-density gas giants in wider orbits. The detection of close-in giant planets around other stars was the first clue that this pattern is not universal and that planets' orbits can change substantially after their formation. Here, we report another violation of the orbitcomposition pattern: two planets orbiting the same star with orbital distances differing by only 10% and densities differing by a factor of 8. One planet is likely a rocky "super-Earth," whereas the other is more akin to Neptune. These planets are 20 times more closely spaced and have a larger density contrast than any adjacent pair of planets in the solar system.

U2 - 10.1126/science.1223269

DO - 10.1126/science.1223269

M3 - Journal article

C2 - 22722249

SN - 0036-8075

VL - 337

SP - 556

EP - 559

JO - Science

JF - Science

IS - 6094

ER -

Kepler-36: a pair of planets with neighboring orbits and dissimilar densities

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