An Earth-sized planet in the habitable zone of a cool star

Elisa V. Quintana; Thomas Barclay; Sean N. Raymond; Jason F. Rowe; Emeline Bolmont; Douglas A. Caldwell; Steve B. Howell; Stephen R. Kane; Daniel Huber; Justin R. Crepp; Jack J. Lissauer; David R. Ciardi; Jeffrey L. Coughlin; Mark E. Everett; Christopher E. Henze; Elliott Horch; Howard Isaacson; Eric B. Ford; Fred C. Adams; Martin Still; Roger C. Hunter; Billy Quarles; Franck Selsis

doi:10.1126/science.1249403

An Earth-sized planet in the habitable zone of a cool star

Elisa V. Quintana, Thomas Barclay, Sean N. Raymond, Jason F. Rowe, Emeline Bolmont, Douglas A. Caldwell, Steve B. Howell, Stephen R. Kane, Daniel Huber, Justin R. Crepp, Jack J. Lissauer, David R. Ciardi, Jeffrey L. Coughlin, Mark E. Everett, Christopher E. Henze, Elliott Horch, Howard Isaacson, Eric B. Ford, Fred C. Adams, Martin StillRoger C. Hunter, Billy Quarles, Franck Selsis

Namur Institute for Complex Systems

Résultats de recherche: Contribution à un journal/une revue › Article › Revue par des pairs

Résumé

The quest for Earth-like planets is a major focus of current exoplanet research. Although planets that are Earth-sized and smaller have been detected, these planets reside in orbits that are too close to their host star to allow liquid water on their surfaces. We present the detection of Kepler-186f, a 1.11 ± 0.14 Earth-radius planet that is the outermost of five planets, all roughly Earth-sized, that transit a 0.47 ± 0.05 solar-radius star. The intensity and spectrum of the star's radiation place Kepler-186f in the stellar habitable zone, implying that if Kepler-186f has an Earth-like atmosphere and water at its surface, then some of this water is likely to be in liquid form.

langue originale	Anglais
Pages (de - à)	277-280
Nombre de pages	4
journal	Science
Volume	344
Numéro de publication	6181
Les DOIs	https://doi.org/10.1126/science.1249403
Etat de la publication	Publié - 1 janv. 2014

Accès au document

10.1126/science.1249403

Autres fichiers et liens

Link to publication in Scopus

Contient cette citation

Quintana, E. V., Barclay, T., Raymond, S. N., Rowe, J. F., Bolmont, E., Caldwell, D. A., Howell, S. B., Kane, S. R., Huber, D., Crepp, J. R., Lissauer, J. J., Ciardi, D. R., Coughlin, J. L., Everett, M. E., Henze, C. E., Horch, E., Isaacson, H., Ford, E. B., Adams, F. C., ... Selsis, F. (2014). An Earth-sized planet in the habitable zone of a cool star. Science, 344(6181), 277-280. https://doi.org/10.1126/science.1249403

@article{97dcd004d9e64ceaa3140eeb8efa0f5d,

title = "An Earth-sized planet in the habitable zone of a cool star",

abstract = "The quest for Earth-like planets is a major focus of current exoplanet research. Although planets that are Earth-sized and smaller have been detected, these planets reside in orbits that are too close to their host star to allow liquid water on their surfaces. We present the detection of Kepler-186f, a 1.11 ± 0.14 Earth-radius planet that is the outermost of five planets, all roughly Earth-sized, that transit a 0.47 ± 0.05 solar-radius star. The intensity and spectrum of the star's radiation place Kepler-186f in the stellar habitable zone, implying that if Kepler-186f has an Earth-like atmosphere and water at its surface, then some of this water is likely to be in liquid form.",

author = "Quintana, {Elisa V.} and Thomas Barclay and Raymond, {Sean N.} and Rowe, {Jason F.} and Emeline Bolmont and Caldwell, {Douglas A.} and Howell, {Steve B.} and Kane, {Stephen R.} and Daniel Huber and Crepp, {Justin R.} and Lissauer, {Jack J.} and Ciardi, {David R.} and Coughlin, {Jeffrey L.} and Everett, {Mark E.} and Henze, {Christopher E.} and Elliott Horch and Howard Isaacson and Ford, {Eric B.} and Adams, {Fred C.} and Martin Still and Hunter, {Roger C.} and Billy Quarles and Franck Selsis",

year = "2014",

month = jan,

day = "1",

doi = "10.1126/science.1249403",

language = "English",

volume = "344",

pages = "277--280",

journal = "Science",

issn = "0036-8075",

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

number = "6181",

}

Quintana, EV, Barclay, T, Raymond, SN, Rowe, JF, Bolmont, E, Caldwell, DA, Howell, SB, Kane, SR, Huber, D, Crepp, JR, Lissauer, JJ, Ciardi, DR, Coughlin, JL, Everett, ME, Henze, CE, Horch, E, Isaacson, H, Ford, EB, Adams, FC, Still, M, Hunter, RC, Quarles, B & Selsis, F 2014, 'An Earth-sized planet in the habitable zone of a cool star', Science, VOL. 344, Numéro 6181, p. 277-280. https://doi.org/10.1126/science.1249403

TY - JOUR

T1 - An Earth-sized planet in the habitable zone of a cool star

AU - Quintana, Elisa V.

AU - Barclay, Thomas

AU - Raymond, Sean N.

AU - Rowe, Jason F.

AU - Bolmont, Emeline

AU - Caldwell, Douglas A.

AU - Howell, Steve B.

AU - Kane, Stephen R.

AU - Huber, Daniel

AU - Crepp, Justin R.

AU - Lissauer, Jack J.

AU - Ciardi, David R.

AU - Coughlin, Jeffrey L.

AU - Everett, Mark E.

AU - Henze, Christopher E.

AU - Horch, Elliott

AU - Isaacson, Howard

AU - Ford, Eric B.

AU - Adams, Fred C.

AU - Still, Martin

AU - Hunter, Roger C.

AU - Quarles, Billy

AU - Selsis, Franck

PY - 2014/1/1

Y1 - 2014/1/1

N2 - The quest for Earth-like planets is a major focus of current exoplanet research. Although planets that are Earth-sized and smaller have been detected, these planets reside in orbits that are too close to their host star to allow liquid water on their surfaces. We present the detection of Kepler-186f, a 1.11 ± 0.14 Earth-radius planet that is the outermost of five planets, all roughly Earth-sized, that transit a 0.47 ± 0.05 solar-radius star. The intensity and spectrum of the star's radiation place Kepler-186f in the stellar habitable zone, implying that if Kepler-186f has an Earth-like atmosphere and water at its surface, then some of this water is likely to be in liquid form.

AB - The quest for Earth-like planets is a major focus of current exoplanet research. Although planets that are Earth-sized and smaller have been detected, these planets reside in orbits that are too close to their host star to allow liquid water on their surfaces. We present the detection of Kepler-186f, a 1.11 ± 0.14 Earth-radius planet that is the outermost of five planets, all roughly Earth-sized, that transit a 0.47 ± 0.05 solar-radius star. The intensity and spectrum of the star's radiation place Kepler-186f in the stellar habitable zone, implying that if Kepler-186f has an Earth-like atmosphere and water at its surface, then some of this water is likely to be in liquid form.

UR - http://www.scopus.com/inward/record.url?scp=84899477291&partnerID=8YFLogxK

U2 - 10.1126/science.1249403

DO - 10.1126/science.1249403

M3 - Article

C2 - 24744370

AN - SCOPUS:84899477291

SN - 0036-8075

VL - 344

SP - 277

EP - 280

JO - Science

JF - Science

IS - 6181

ER -

An Earth-sized planet in the habitable zone of a cool star

Résumé

Accès au document

Autres fichiers et liens

Empreinte digitale

Contient cette citation