HAT-P-16b: A 4 MJ planet transiting a bright star on an eccentric orbit

L. A. Buchhave; G. A. Bakos; J. D. Hartman; G. Torres; G. Kovács; D. W. Latham; R. W. Noyes; G. A. Esquerdo; M. Everett; A. W. Howard; G. W. Marcy; D. A. Fischer; J. A. Johnson; J. Andersen; G. Furész; G. Perumpilly; D. D. Sasselov; R. P. Stefanik; B. Béky; J. Lázár; I. Papp; P. Sári

doi:10.1088/0004-637X/720/2/1118

HAT-P-16b: A 4 M_J planet transiting a bright star on an eccentric orbit

L. A. Buchhave, G. A. Bakos, J. D. Hartman, G. Torres, G. Kovács, D. W. Latham, R. W. Noyes, G. A. Esquerdo, M. Everett, A. W. Howard, G. W. Marcy, D. A. Fischer, J. A. Johnson, J. Andersen, G. Furész, G. Perumpilly, D. D. Sasselov, R. P. Stefanik, B. Béky, J. LázárI. Papp, P. Sári

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

253 Scopus citations

Abstract

We report the discovery of HAT-P-16b, a transiting extrasolar planet orbiting the V = 10.8 mag F8 dwarf GSC 2792-01700, with a period P = 2.775960 ± 0.000003 days, transit epoch T_c = 2455027.59293 ± 0.00031 (BJD¹⁰), and transit duration 0.1276 ± 0.0013 days. The host star has a mass of 1.22 ± 0.04 M_⊙, radius of 1.24 ± 0.05 R_⊙, effective temperature 6158 ± 80 K, and metallicity [Fe/H] = +0.17 ± 0.08. The planetary companion has a mass of 4.193 ± 0.094 MJ and radius of 1.289 ± 0.066 RJ, yielding a mean density of 2.42 ± 0.35 gcm-3. Comparing these observed characteristics with recent theoretical models, we find that HAT-P-16b is consistent with a 1 Gyr H/He-dominated gas giant planet. HAT-P-16b resides in a sparsely populated region of the mass-radius diagram and has a non-zero eccentricity of e = 0.036 with a significance of 10σ.

Original language	English (US)
Pages (from-to)	1118-1125
Number of pages	8
Journal	Astrophysical Journal
Volume	720
Issue number	2
DOIs	https://doi.org/10.1088/0004-637X/720/2/1118
State	Published - Sep 10 2010
Externally published	Yes

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics
Space and Planetary Science

Keywords

Planetary systems
Stars: individual (HAT-P-16, GSC 2792-01700)
Techniques: photometric
Techniques: spectroscopic

Access to Document

10.1088/0004-637X/720/2/1118

Cite this

Buchhave, L. A., Bakos, G. A., Hartman, J. D., Torres, G., Kovács, G., Latham, D. W., Noyes, R. W., Esquerdo, G. A., Everett, M., Howard, A. W., Marcy, G. W., Fischer, D. A., Johnson, J. A., Andersen, J., Furész, G., Perumpilly, G., Sasselov, D. D., Stefanik, R. P., Béky, B., ... Sári, P. (2010). HAT-P-16b: A 4 M_J planet transiting a bright star on an eccentric orbit. Astrophysical Journal, 720(2), 1118-1125. https://doi.org/10.1088/0004-637X/720/2/1118

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title = "HAT-P-16b: A 4 MJ planet transiting a bright star on an eccentric orbit",

abstract = "We report the discovery of HAT-P-16b, a transiting extrasolar planet orbiting the V = 10.8 mag F8 dwarf GSC 2792-01700, with a period P = 2.775960 ± 0.000003 days, transit epoch Tc = 2455027.59293 ± 0.00031 (BJD10), and transit duration 0.1276 ± 0.0013 days. The host star has a mass of 1.22 ± 0.04 M⊙, radius of 1.24 ± 0.05 R⊙, effective temperature 6158 ± 80 K, and metallicity [Fe/H] = +0.17 ± 0.08. The planetary companion has a mass of 4.193 ± 0.094 MJ and radius of 1.289 ± 0.066 RJ, yielding a mean density of 2.42 ± 0.35 gcm-3. Comparing these observed characteristics with recent theoretical models, we find that HAT-P-16b is consistent with a 1 Gyr H/He-dominated gas giant planet. HAT-P-16b resides in a sparsely populated region of the mass-radius diagram and has a non-zero eccentricity of e = 0.036 with a significance of 10σ.",

keywords = "Planetary systems, Stars: individual (HAT-P-16, GSC 2792-01700), Techniques: photometric, Techniques: spectroscopic",

author = "Buchhave, {L. A.} and Bakos, {G. A.} and Hartman, {J. D.} and G. Torres and G. Kov{\'a}cs and Latham, {D. W.} and Noyes, {R. W.} and Esquerdo, {G. A.} and M. Everett and Howard, {A. W.} and Marcy, {G. W.} and Fischer, {D. A.} and Johnson, {J. A.} and J. Andersen and G. Fur{\'e}sz and G. Perumpilly and Sasselov, {D. D.} and Stefanik, {R. P.} and B. B{\'e}ky and J. L{\'a}z{\'a}r and I. Papp and P. S{\'a}ri",

year = "2010",

month = sep,

day = "10",

doi = "10.1088/0004-637X/720/2/1118",

language = "English (US)",

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Buchhave, LA, Bakos, GA , Hartman, JD, Torres, G, Kovács, G, Latham, DW, Noyes, RW, Esquerdo, GA, Everett, M, Howard, AW, Marcy, GW, Fischer, DA, Johnson, JA, Andersen, J, Furész, G, Perumpilly, G, Sasselov, DD, Stefanik, RP, Béky, B, Lázár, J, Papp, I & Sári, P 2010, 'HAT-P-16b: A 4 M_J planet transiting a bright star on an eccentric orbit', Astrophysical Journal, vol. 720, no. 2, pp. 1118-1125. https://doi.org/10.1088/0004-637X/720/2/1118

TY - JOUR

T1 - HAT-P-16b

T2 - A 4 MJ planet transiting a bright star on an eccentric orbit

AU - Buchhave, L. A.

AU - Bakos, G. A.

AU - Hartman, J. D.

AU - Torres, G.

AU - Kovács, G.

AU - Latham, D. W.

AU - Noyes, R. W.

AU - Esquerdo, G. A.

AU - Everett, M.

AU - Howard, A. W.

AU - Marcy, G. W.

AU - Fischer, D. A.

AU - Johnson, J. A.

AU - Andersen, J.

AU - Furész, G.

AU - Perumpilly, G.

AU - Sasselov, D. D.

AU - Stefanik, R. P.

AU - Béky, B.

AU - Lázár, J.

AU - Papp, I.

AU - Sári, P.

PY - 2010/9/10

Y1 - 2010/9/10

N2 - We report the discovery of HAT-P-16b, a transiting extrasolar planet orbiting the V = 10.8 mag F8 dwarf GSC 2792-01700, with a period P = 2.775960 ± 0.000003 days, transit epoch Tc = 2455027.59293 ± 0.00031 (BJD10), and transit duration 0.1276 ± 0.0013 days. The host star has a mass of 1.22 ± 0.04 M⊙, radius of 1.24 ± 0.05 R⊙, effective temperature 6158 ± 80 K, and metallicity [Fe/H] = +0.17 ± 0.08. The planetary companion has a mass of 4.193 ± 0.094 MJ and radius of 1.289 ± 0.066 RJ, yielding a mean density of 2.42 ± 0.35 gcm-3. Comparing these observed characteristics with recent theoretical models, we find that HAT-P-16b is consistent with a 1 Gyr H/He-dominated gas giant planet. HAT-P-16b resides in a sparsely populated region of the mass-radius diagram and has a non-zero eccentricity of e = 0.036 with a significance of 10σ.

AB - We report the discovery of HAT-P-16b, a transiting extrasolar planet orbiting the V = 10.8 mag F8 dwarf GSC 2792-01700, with a period P = 2.775960 ± 0.000003 days, transit epoch Tc = 2455027.59293 ± 0.00031 (BJD10), and transit duration 0.1276 ± 0.0013 days. The host star has a mass of 1.22 ± 0.04 M⊙, radius of 1.24 ± 0.05 R⊙, effective temperature 6158 ± 80 K, and metallicity [Fe/H] = +0.17 ± 0.08. The planetary companion has a mass of 4.193 ± 0.094 MJ and radius of 1.289 ± 0.066 RJ, yielding a mean density of 2.42 ± 0.35 gcm-3. Comparing these observed characteristics with recent theoretical models, we find that HAT-P-16b is consistent with a 1 Gyr H/He-dominated gas giant planet. HAT-P-16b resides in a sparsely populated region of the mass-radius diagram and has a non-zero eccentricity of e = 0.036 with a significance of 10σ.

KW - Planetary systems

KW - Stars: individual (HAT-P-16, GSC 2792-01700)

KW - Techniques: photometric

KW - Techniques: spectroscopic

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U2 - 10.1088/0004-637X/720/2/1118

DO - 10.1088/0004-637X/720/2/1118

M3 - Article

AN - SCOPUS:78049525598

SN - 0004-637X

VL - 720

SP - 1118

EP - 1125

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

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