Kepler-7b: a transiting planet with unusually low density

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Standard

Kepler-7b : a transiting planet with unusually low density. / Latham...[et al.], David W.; Borucki, W.J.; Koch, D.G.; Buchhave, Lars C. Astrup.

I: The Astrophysical Journal Letters, Bind 713, Nr. 2, 20.04.2010, s. L140-L144.

Publikation: Bidrag til tidsskrift › Tidsskriftartikel › Forskning › fagfællebedømt

Harvard

Latham...[et al.], DW, Borucki, WJ, Koch, DG & Buchhave, LCA 2010, 'Kepler-7b: a transiting planet with unusually low density', The Astrophysical Journal Letters, bind 713, nr. 2, s. L140-L144. https://doi.org/10.1088/2041-8205/713/2/L140

APA

Latham...[et al.], D. W., Borucki, W. J., Koch, D. G., & Buchhave, L. C. A. (2010). Kepler-7b: a transiting planet with unusually low density. The Astrophysical Journal Letters, 713(2), L140-L144. https://doi.org/10.1088/2041-8205/713/2/L140

Vancouver

Latham...[et al.] DW, Borucki WJ, Koch DG, Buchhave LCA. Kepler-7b: a transiting planet with unusually low density. The Astrophysical Journal Letters. 2010 apr. 20;713(2):L140-L144. https://doi.org/10.1088/2041-8205/713/2/L140

Author

Latham...[et al.], David W. ; Borucki, W.J. ; Koch, D.G. ; Buchhave, Lars C. Astrup. / Kepler-7b : a transiting planet with unusually low density. I: The Astrophysical Journal Letters. 2010 ; Bind 713, Nr. 2. s. L140-L144.

Bibtex

@article{7e4e42660340412db43d11b41a6df834,
title = "Kepler-7b: a transiting planet with unusually low density",
abstract = "We report on the discovery and confirmation of Kepler-7b, a transiting planet with unusually low density. The mass is less than half that of Jupiter, M P = 0.43 M J, but the radius is 50% larger, R P = 1.48 R J. The resulting density, ¿P = 0.17 g cm–3, is the second lowest reported so far for an extrasolar planet. The orbital period is fairly long, P = 4.886 days, and the host star is not much hotter than the Sun, T eff = 6000 K. However, it is more massive and considerably larger than the Sun, M = 1.35 M and R = 1.84 R , and must be near the end of its life on the main sequence ",
author = "{Latham...[et al.]}, {David W.} and W.J. Borucki and D.G. Koch and Buchhave, {Lars C. Astrup}",
year = "2010",
month = apr,
day = "20",
doi = "10.1088/2041-8205/713/2/L140",
language = "English",
volume = "713",
pages = "L140--L144",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "2",

}

RIS

TY - JOUR

T1 - Kepler-7b

T2 - a transiting planet with unusually low density

AU - Latham...[et al.], David W.

AU - Borucki, W.J.

AU - Koch, D.G.

AU - Buchhave, Lars C. Astrup

PY - 2010/4/20

Y1 - 2010/4/20

N2 - We report on the discovery and confirmation of Kepler-7b, a transiting planet with unusually low density. The mass is less than half that of Jupiter, M P = 0.43 M J, but the radius is 50% larger, R P = 1.48 R J. The resulting density, ¿P = 0.17 g cm–3, is the second lowest reported so far for an extrasolar planet. The orbital period is fairly long, P = 4.886 days, and the host star is not much hotter than the Sun, T eff = 6000 K. However, it is more massive and considerably larger than the Sun, M = 1.35 M and R = 1.84 R , and must be near the end of its life on the main sequence

AB - We report on the discovery and confirmation of Kepler-7b, a transiting planet with unusually low density. The mass is less than half that of Jupiter, M P = 0.43 M J, but the radius is 50% larger, R P = 1.48 R J. The resulting density, ¿P = 0.17 g cm–3, is the second lowest reported so far for an extrasolar planet. The orbital period is fairly long, P = 4.886 days, and the host star is not much hotter than the Sun, T eff = 6000 K. However, it is more massive and considerably larger than the Sun, M = 1.35 M and R = 1.84 R , and must be near the end of its life on the main sequence

U2 - 10.1088/2041-8205/713/2/L140

DO - 10.1088/2041-8205/713/2/L140

M3 - Journal article

VL - 713

SP - L140-L144

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

ER -

ID: 32928405