Список экзопланет в созвездии Возничего
Список экзопланет в созвездии Возничего содержит 16 экзопланет в 16 разных планетных системах, находящихся в соответствующем созвездии. Перечислены только экзопланеты со статусом Confirmed в EPE.
Учёные постоянно совершают открытия, поэтому список может быть неполон.
Оценить зону обитаемости можно на основе светимости звезды.
Система | # | Удалённость св. лет |
Светимость L⊙ |
Большая полуось а.e. |
Эксцентриситет | Период обращения сут |
Масса MJ |
Пр. |
---|---|---|---|---|---|---|---|---|
HD 33632 | b | 87 | 23,6 ± 3,2 | 0,12 | 39082 ± 7670 | 50 ± 5,6 | EPEDR2[1] | |
TOI-1693 | b | 100 | 0,02 | 1,77 | 0,009 ± 0,007 | EPE[2] | ||
HD 40979 | b | 111 | 1,96 | 0,85 ± 0,01 | 0,25 | 264,15 ± 0,23 | >4,01 ± 0,13 | EPEDR2[3] |
HD 42012 | b | 120 | 0,537 | 1,67 ± 0,05 | 0 | 857,5 ± 6,3 | >1,6 ± 0,1 | EPEDR2[4] |
HD 49674 | b | 141 | 0,952 | 0,06 | 0,05 | 4,95 | >0,1 | EPEDR2[5][6] |
HD 45350 | b | 153 | 1,383 | 1,92 ± 0,07 | 0,78 | 963,6 ± 3,4 | >1,79 ± 0,14 | EPEDR2[7] |
HD 43691 | b | 280 | 3,747 | 0,24 ± 0,01 | 0,09 | 37 | >2,57 ± 0,3 | EPEDR2[8] |
HD 42176 | b | 439 | 4,885 | 0,05 | 0,19 | 4,11 | 1,486 ± 0,088 | EPEDR2[9] |
HD 33643 | b | 448 | 5,715 | 0,04 | 2,73 | >1,28 ± 0,18 | EPEDR2[10][11] | |
AB Возничего | b | 531 | 93,9 ± 50 | 0,4 | 9 ± 17 | EPEDR2[12][13] | ||
HAT-P-61 | b | 1119 | 0,03 | 1,9 | 1,057 ± 0,07 | EPE[14] | ||
HAT-P-62 | b | 1152 | 0,04 | 0,1 | 2,65 | 0,761 ± 0,088 | EPE[14] | |
TOI-2570 | b | 1180 | 0,04 | 0 | 2,99 | 82 ± 0,065 | EPE[15] | |
WASP-12 | b | 1411 | 3,435 | 0,02 | 0 | 1,09 | >1,46 ± 0,075 | EPEDR2[16][17][18][19] |
HAT-P-9 | b | 5104 | 0,05 | 0 | 3,92 | >0,748 ± 0,063 | EPEDR2[20][21][22] | |
PSR J0636+5129 | b | 0,07 | >8 | EPE[23] |
Примечания
- ↑ Trent J. Dupuy (2021), Improved Dynamical Masses for Six Brown Dwarf Companions Using Hipparcos and Gaia EDR3, The Astronomical Journal Т. 162 (6): 301
- ↑ Ethan Kruse (2022), Validation of 13 Hot and Potentially Terrestrial TESS Planets, The Astronomical Journal Т. 163 (2): 99
- ↑ Harold F. Levison (2009), A Search for Multi-Planet Systems Using the Hobby-Eberly Telescope, The Astrophysical Journal Supplement Series Т. 182 (1): 97–119
- ↑ Claire Moutou (2017), The SOPHIE search for northern extrasolar planets. XII. Three giant planets suitable for astrometric mass determination with Gaia, Astronomy and Astrophysics Т. 601: 9–9
- ↑ Jason Wright (2007), Four New Exoplanets and Hints of Additional Substellar Companions to Exoplanet Host Stars, Letters of the Astrophysical Journal Т. 657 (1): 533–545, <https://iopscience.iop.org/article/10.1086/510553/pdf>
- ↑ Ji Wang (2011), On the eccentricity distribution of short-period single-planet systems, Monthly Notices of the Royal Astronomical Society Т. 418 (3): 1822–1833
- ↑ Harold F. Levison (2007), Dynamical and Observational Constraints on Additional Planets in Highly Eccentric Planetary Systems, The Astronomical Journal Т. 134 (3): 1276–1284
- ↑ Joshua Pepper (2020), Orbital Refinement and Stellar Properties for the HD 9446, HD 43691, and HD 179079 Planetary Systems, The Astronomical Journal Т. 159 (5): 197
- ↑ Mark Trueblood (2012), KELT-2Ab: A HOT JUPITER TRANSITING THE BRIGHT ( V = 8.77) PRIMARY STAR OF A BINARY SYSTEM, Letters of the Astrophysical Journal Т. 756 (2): 39, <https://iopscience.iop.org/article/10.1088/2041-8205/756/2/L39/pdf>
- ↑ Critical Analysis of Tess Transit Photometric Data: Improved Physical Properties for Five Exoplanets, The Astronomical Journal Т. 162 (5): 221, 2021
- ↑ Matthew Penny (2015), KELT-7b: A HOT JUPITER TRANSITING A BRIGHTV= 8.54 RAPIDLY ROTATING F-STAR, The Astronomical Journal Т. 150 (1): 12
- ↑ Peter G. Tuthill (2022), Images of embedded Jovian planet formation at a wide separation around AB Aurigae, Nature Astronomy Т. 6 (6): 751-759
- ↑ Neil T. Zimmerman (2008), The Solar‐System‐Scale Disk around AB Aurigae, The Astrophysical Journal Т. 679 (2): 1574–1581, <https://iopscience.iop.org/article/10.1086/587778/pdf>
- ↑ 14,0 14,1 Waqas Bhatti (2021), HAT-P-58b–HAT-P-64b: Seven Planets Transiting Bright Stars*, The Astronomical Journal Т. 162 (1): 7
- ↑ Stephen R. Kane (2022), The TESS Grand Unified Hot Jupiter Survey. I. Ten TESS Planets, The Astronomical Journal Т. 164 (2): 70
- ↑ Orbital period modulation in hot Jupiter systems, Monthly Notices of the Royal Astronomical Society Т. 497 (3): 3911-3924, 2020
- ↑ Björn Benneke, TESS Revisits WASP-12: Updated Orbital Decay Rate and Constraints on Atmospheric Variability
- ↑ Roberto Sanchis-Ojeda (2011), The transit light-curve project. XIV. Confirmation of anomalous radii for the exoplanets TrES-4b, HAT-P-3b, and WASP-12b, The Astronomical Journal Т. 141 (6): 179
- ↑ Keivan Stassun (2017), Transit timing variation measurements of WASP-12b and Qatar-1b: no evidence of additional planets, The Astronomical Journal Т. 153 (2): 78–78
- ↑ Tsevi Mazeh (2008), HAT-P-9b: A Low Density Planet Transiting a Moderately Faint F star, The Astrophysical Journal Т. 690 (2): 1393–1400, <https://iopscience.iop.org/article/10.1088/0004-637X/690/2/1393/pdf>
- ↑ Isabelle Boisse (2011), Spin-orbit inclinations of the exoplanetary systems HAT-P-8b, HAT-P-9b, HAT-P-16b, and HAT-P-23b, Astronomy and Astrophysics Т. 533: 113–113
- ↑ Transiting Exoplanet Monitoring Project (TEMP). V. Transit follow up for HAT-P-9b, HAT-P-32b, and HAT-P-36b, The Astronomical Journal Т. 157: 82–82, 2019
- ↑ Renée Spiewak (2016), Ordinary x-rays from three extraordinary millisecond pulsars: XMM-Newton observations of PSRs J0337+1715, J0636+5129, and J0645+5158, The Astrophysical Journal Т. 822 (1): 37–37, <https://iopscience.iop.org/article/10.3847/0004-637X/822/1/37/pdf>