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LTT 1445 Ab

LTT 1445 Ab
Discovery
Discovery date2019
Transit
Orbital characteristics
0.022
5.4 d
StarLTT 1445 A
Physical characteristics
1.18 R🜨
Mass2.87 ME

LTT 1445 Ab is an exoplanet that was discovered in 2019. The planet is located about 22 light years away from Earth and takes 5 days to orbit its star, which in turn orbits two sibling stars, making a total of three stars in the system.

Discovery

This superheated planet, about 1.4 times the size of Earth, has a sky one fortress bigger than Star Wars' Tatooine -- three stars instead of two. It was found by a team at the Harvard Center for Astrophysics using data from the TESS space telescope on July 26, 2019.

Key facts

LTT 1445 Ab, apparently a rocky planet, takes only five days to orbit its star β€”a "year" on this world, which is about 22.5 light-years from Earth. Its extremely close orbit helps explain why its surface heats to temperatures on the order of 320 degrees Fahrenheit (160 Celsius), comparable to a preheated oven.[1]

Details

While the planet itself remains in a presumably stable orbit around its star, that star also orbits at greater distances around two sister stars that are locked in close orbit around each other. This is not the first triple star system to contain at least one planet. In fact, our nearest stellar neighbor is Proxima Centauri, which orbits a more distant pair, Alpha Centauri A and B. Proxima Centauri is only 4.25 light-years from Earth. It is orbited by Proxima Centauri b, a small, possibly rocky world estimated to take 11 days to orbit its star. According to the TESS data, scientists believe the planet is rocky, about a third larger than Earth, and at most about 8 times more massive than Earth.

Interesting facts

All three stars in the LTT 1445 system are red dwarfs, which are cooler and burn much longer than large yellow stars like our Sun. This planet is also the second-closest known planet to "pass" its starβ€”that is, LTT 1445 Ab's orbit is tilted at just the right angle to pass across its star from our perspective. The "transit" observing method allows space telescopes like TESS to detect planets orbiting other stars by the shadows they cast, the tiny dip in starlight as the planet transits. [2]

The closest transiting planetary system discovered so far is HD 219134 bc, which is about 21 light-years away.

"If you're standing on the surface of this planet, there are three suns in the sky, but two of them are pretty far away and look small," co-author Jennifer Winters, an astronomer at the Harvard-Smithsonian Center for Astrophysics, told New Scientist. "They are like two red ominous eyes in the sky."

Possible atmosphere

But what is particularly special about it is something that scientists cannot yet characterize, but will soon be able to characterize: its atmosphere. Because the stars in question are red dwarfs that are quite close to Earth, and because the system is arranged so that the planet passes between the stars and Earth, scientists may actually be able to see any gases surrounding the planet with telescopes on earth.[3]

In 2022, a planetary transmission spectrum has showed no evidence for the atmosphere, although atmosphere with high altitude hazes cannot be ruled out yet.[4]

References

  1. ^ Brennan, Pat. "Discovery Alert: Rocky Planet Swelters Under Three Red Suns". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 2022-08-04.
  2. ^ Winters, Jennifer G.; et al. (October 2019). "Three Red Suns in the Sky: A Transiting, Terrestrial Planet in a Triple M-dwarf System at 6.9 pc". The Astronomical Journal. 158 (4): 158 152. doi:10.3847/1538-3881/ab364d. hdl:1721.1/124706. S2CID 195584444. Retrieved 9 July 2022.{{cite journal}}: CS1 maint: unflagged free DOI (link)
  3. ^ Meghan, Bartels (2019-07-26). "This Newfound Alien Planet Has 3 Suns". Space.com. Retrieved 2022-08-04.
  4. ^ Diamond-Lowe, Hannah; Mendonca, Joao M.; Charbonneau, David; Buchhave, Lars A. (2022), Ground-based Optical Transmission Spectroscopy of the Nearby Terrestrial Exoplanet LTT 1445Ab, arXiv:2210.11809

BEBOP-1c

KELT-24

KELT-24
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cygnus
Right ascension 10h 47m 38.17s
Declination +71° 39′ 20.62″
Characteristics
Evolutionary stage main sequence star
Spectral type F7V
Variable type planetary transit
Astrometry
Proper motion (ΞΌ) RA: -56.1837 Β± 0.0532497 mas/yr
Dec.: -34.8076 Β± 0.0642398 mas/yr
Parallax (Ο€)10.332 Β± 0.0332707 mas
Details
Mass1.30 M☉
Radius1.52 R☉
Luminosity0.565 L☉
Temperature6415 K
Metallicity [Fe/H]-0.090 Fe dex
Age2.8 Gyr
Other designations
MASCARA-3

KELT-24, also known as MASCARA-3, is a star in the constellation of Ursa Major.

Planetary system

In 2017, the discovery of the Hot Jupiter KELT-24b was announced. TESS data confirmed that no additional companions are orbiting this star. [1]


The KELT-24 planetary system
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b 5.18 MJ 0.06969 5.6 0.08 83.11Β° 1.272 RJ

References

  1. ^ Maciejewski, G. (2020), "Search for Planets in Hot Jupiter Systems with Multi-Sector TESS Photometry. I. No Companions in Planetary Systems KELT-18, KELT-23, KELT-24, Qatar-8, WASP-62, WASP-100, WASP-119, and WASP-126", Acta Astronomica, 70 (3): 181, arXiv:2010.11977, Bibcode:2020AcA....70..181M, doi:10.32023/0001-5237/70.3.2, S2CID 225061977

Reference Testing 1

[1]

Reference Testing 2

[2]

Reference Testing 3

[3]

Reference Testing 4

[4]

Reference Testing 5

[5]


(12345) 1993 FT8

References

  1. ^ "The Extrasolar Planet Encyclopaedia β€” CoRoT-26 b". exoplanet.eu. Retrieved 10 September 2023.
  2. ^ "The Extrasolar Planet Encyclopaedia β€” TOI-849 b". exoplanet.eu. Retrieved 11 September 2023.
  3. ^ "The Extrasolar Planet Encyclopaedia β€” CFHTWIR-Oph 98 b". exoplanet.eu. Retrieved 11 September 2023.
  4. ^ "The Extrasolar Planet Encyclopaedia β€” HD 202772 Ab". exoplanet.eu. Retrieved 11 September 2023.
  5. ^ "The Extrasolar Planet Encyclopaedia β€” TOI-4342 b". exoplanet.eu. Retrieved 11 September 2023.

CoRoT-20

CoRoT-20
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Monoceros
Right ascension 06h 30m 52,900s
Declination +00° 13′ 36.85″
Characteristics
Evolutionary stage main sequence star
Spectral type G2V
Variable type planetary transit
Astrometry
Details
Mass1.14 M☉
Radius1.02 R☉
Temperature5880 K
Age100 million years
Other designations
2MASS J06305289+0013369

CoRoT-20 is a star, which is located in the constellation Monoceros at a distance of about 4011 light years from us. The star is orbited by at least two planets.

Characteristics

CoRoT-20 is a very young star of 14.66 magnitude by astronomical standards. Its age is estimated at approximately 100 million years[1]. In terms of mass and radius, it is almost identical to our Sun. Its surface temperature is about 5880 kelvins. CoRoT-20 got its name thanks to the space telescope CoRoT, which discovered its two planets.

Planetary system

In 2011, a group of astronomers working within the CoRoT program announced[1] the discovery of the planet CoRoT-20b and CoRoT-20c in this system. It is a hot gas giant, more than four times the mass of Jupiter. However, the planet's radius is only 84% of Jupiter's, which indicates an average high density. CoRoT-20b and c both orbit close to its parent star - at a distance of 0.09 AU The discovery of the planet was made by transit method.

The CoRoT-20 planetary system[2]
Companion
(in order from star) 		Mass Semimajor axis
(AU) 		Orbital period
(days) 		Eccentricity Inclination Radius
b 4.3 MJ 0.09 β€” 0.59 β€” β€”
c 17 MJ 2.9 β€” 0.6 β€” β€”

References

  1. ^ a b M. Deleuil, A.S. Bonomo, S. Ferraz-Mello, A. Erikson, F. Bouchy, M. Havel, S. Aigrain, J.-M. Almenara, R. Alonso, M. Auvergne, A. Baglin, P. Barge, P. BordΓ©, H. Bruntt, J. Cabrera, S. Carpano, C. Cavarroc, Sz. Csizmadia, C. Damiani, H.J. Deeg, R. Dvorak, M. Fridlund, G. HΓ©brard, D. Gandolfi, M. Gillon, E. Guenther, T. Guillot, A. Hatzes, L. Jorda, A. LΓ©ger, H. Lammer, T. Mazeh, C. Moutou, M. Ollivier, A. Ofir, H. Parviainen, D. Queloz, H. Rauer, A. RodrΓ­guez, D. Rouan, A. Santerne, J. Schneider, L. Tal-Or, B. Tingley, J. Weingrill, G. Wuchterl. "XX. CoRoT-20b: A very high density, high eccentricity transiting giant planet". Arxiv.org. Archived from the original on 2012-09-01. Retrieved 2011-10-27. {{cite web}}: Cite has empty unknown parameter: |description= (help); Unknown parameter |datepublished= ignored (help)CS1 maint: multiple names: authors list (link)
  2. ^ "CoRoT-20 Planets in the system". Retrieved February 25, 2019.

CFHTWIR-Oph 98 b

CFHTWIR-Oph 98 b
Discovery
Discovery date2019
Direct imaging
Orbital characteristics
200 AU
Eccentricity0
22027.4 y
StarCFHTWIR-Oph 98 A
Physical characteristics
1.86 RJ
Mass7.8 MJ

CFHTWIR-Oph 98 b is a Super-Jupiter exoplanet that orbits CFHTWIR-Oph 98 A, a M-type star. [1]

Formation

It orbits a star but its formation as an exoplanet is challenging or impossible.[2] If it’s formation scenario is known, it may explain the formation of Planet Nine.

References

  1. ^ "The Extrasolar Planet Encyclopaedia β€” CFHTWIR-Oph 98 b". exoplanet.eu. Retrieved 11 September 2023.
  2. ^ Fontanive, ClΓ©mence; Allers, Katelyn N.; Pantoja, Blake; Biller, Beth; Dubber, Sophie; Zhang, Zhoujian; Dupuy, Trent; Liu, Michael C.; Albert, LoΓ―c (2020-12-01). "A Wide Planetary-mass Companion to a Young Low-mass Brown Dwarf in Ophiuchus". The Astrophysical Journal. 905: L14. doi:10.3847/2041-8213/abcaf8. ISSN 0004-637X.{{cite journal}}: CS1 maint: unflagged free DOI (link)

ΞΌΒ²

List of exoplanets that host stars are visible to the naked eye: Bayer designations

Star Exoplanet Mass
(MJ) 		Semimajor axis
(AU) 		Orbital period Discovered Discovery method Reference
Ξ± Arietis b 1.8Β±0.2 1.2 380.8Β±0.3 d 2011 Radial velocity [1]
Ξ± Tauri b 5.8Β±0.7 1.46Β±0.27 628.96Β±0.9 d 2015 Radial velocity [2]
Ξ² Cancri b 7.8Β±0.8 1.7Β±0.1 605.2Β±4 d 2014 Radial velocity [3]
Ξ² Pictoris b 11.729+1.175
βˆ’2.135 		10.018+0.082
βˆ’0.076 		23.593+0.248
βˆ’0.209 d 		2008 Infrared [4]
Ξ² Pictoris c 10.139+1.175
βˆ’1.031 		2.680+0.016
βˆ’0.015 		3.266+0.015
βˆ’0.012 d 		2020 Direct imaging [5]
Ξ² Ursae Minoris b 6.1Β±1.0 1.4Β±0.1 522.3Β±2.7 d 2014 Radial velocity [6]
Ξ³ Cephei A b 9.4+0.7
βˆ’1.1 		2.05Β±0.06 903.3Β±1.5 d 2002 Doppler spectroscopy [7]
Ξ³1 Leonis b ? 1.19 429 d 2009 Radial velocity [8]
Ξ³ Librae b 1.02 1.24 415.2 d 2018 Radial velocity [9]
Ξ³ Librae c 4.58 2.17 964.6Β±3.1 d 2018 Radial velocity [10]
Ξ³ Piscium b 1.34+0.02
βˆ’0.31 		1.32+0.05
βˆ’0.08 		555.1+6.0
βˆ’2.5 d 		2021 Radial velocity [11]
Ξ΅ Coronae Borealis b 6.7Β±0.3 1.3 417.9Β±0.5 d 2012 Radial velocity [12]
Ξ΅ Eridani b 0.63+0.12
βˆ’0.04 		3.52Β±0.04 2775Β±5 d 2000 Doppler spectroscopy [13]
Ξ΅ Indi A b 3.0Β±0.1 8.8+0.2
βˆ’0.1 		10932+266
βˆ’228 d 		2018 Radial velocity [14]
Ξ΅ Tauri b 7.6Β±0.2 1.93Β±0.03 645.5Β±5.3 d 2007 Doppler spectroscopy [15]
ΞΉ Draconis b 16.4+9.3
βˆ’4 		1.453Β±0.026 510.854Β±0.013 d 2002 Doppler spectroscopy [16]
ΞΉ Draconis c 17.0+13
βˆ’5.4 		19.4+10
βˆ’7.7 		68+60
βˆ’36 d 		2021 Radial velocity [17]
ΞΊ Andromedae b 13+12
βˆ’2 		57Β±133 242Β±900 y 2012 Direct imaging [18]
ΞΊ Coronae Borealis b 1.811Β±0.057 2.65Β±0.13 1285Β±14 2012 Radial velocity [19]
ΞΌ Arae b 1.65Β±0.009 1.522Β±0.001 643.25Β±0.90 d 2000 Doppler spectroscopy [20]
ΞΌ Arae c 0.032Β±0.002 0.09094Β±0.000005 9.6386Β±0.0015 d 2004 Radial velocity [21]
ΞΌ Arae d 0.448Β±0.011 0.9210Β±0.0015 1310.55Β±0.83 d 2006 Doppler spectroscopy [22]
ΞΌ Arae e 5.235 4205.8Β±758.9 d 2002 Radial velocity [23]
ΞΌ Leonis b 2.4Β±0.4 1.1Β±0.1 357.8Β±1.2 d 2014 Radial velocity [24]
ΞΌ2 Scorpii b 14.4Β±0.8 242.4+114.5
βˆ’52.1 		? 2022 Direct imaging [25]
Ξ½ Octantis A b 2.1059 1.276 414.8 d 2021 Radial velocity [26]
Ξ½ Ophiuchi b 81.7Β±22.2 1.803 530.73Β±0.10 d 2012 Radial velocity [27]
Ξ½ Ophiuchi c 92Β±24.7 6.022 3188.95Β±6.26d 2012 Radial velocity [28]
ΞΎ Aquilae b 2.8 0.68 136.75Β±0.25 2008 Radial velocity [29]
ΞΏ Coronae Borealis b 1.5 0.83 187.83Β±0.54 d 2012 Radial velocity [30]
ΞΏ Ursae Majoris b 4.1 3.9 1630Β±35 d 2012 Radial velocity [31]
Ο€ Mensae b 12.325+1.192
βˆ’1.384 		3.311+0.134
βˆ’0.148 		5.719Β±0.001 y 2001 Doppler spectroscopy [32]
Ο€ Mensae c 3.63Β±0.38 0.06839Β±0.0005 6.267852Β±0.000016 d 2014 Transit [33]
Ο€ Mensae d 3.63Β±0.38 ? 124.64+0.48
βˆ’0.52 d 		2023 Radial velocity [34]
ρ1 Cancri b 0.824±0.007 0.115±0.0000011 14.65162±0.0007 d 1996 Radial velocity [35]
ρ1 Cancri c 51.2±1.3 0.240±0.00005 44.3446±0.007 d 2002 Radial velocity [36]
ρ1 Cancri d 3.12±0.1 5.77±0.11 5218±230 d 2002 Radial velocity [37]
ρ1 Cancri e 7.99+0.32
βˆ’0.33 		0.01544Β±0.00005 17.67711 h 2004 Radial velocity [38]
ρ1 Cancri f 7.70±0.08 0.781±0.007 260±1.1 d 2005 Doppler spectroscopy [39]
ρ Coronae Borealis b 1.093±0.023 0.2245+0.0023
βˆ’0.0024 		39.8438Β±0.0027 d 1997 Radial velocity [40]
ρ Coronae Borealis c 28.2±1.5 0.4206+0.0044
βˆ’0.0024 		102.19+0.27
βˆ’0.22 d 		2016 Radial velocity [41]
ρ Coronae Borealis d 21.6±2.5 0.827±0.011 282.2+2.2
βˆ’3.7 d 		2023 Radial velocity [42]
ρ Coronae Borealis e 3.79+0.53
βˆ’0.54 		0.1061Β±0.0011 12.949Β±0.014 d 2023 Radial velocity [43]
Ο„ BoΓΆtis b 5.5Β±6 0.0481 3.312463Β±0.000014d 1996 Radial velocity [44]
Ο„ Ceti e 3.93+0.83
βˆ’0.64 		0.538Β±0.006 162.87+1.08
βˆ’0.46 d 		2012 Radial velocity [45]
Ο„ Ceti f 3.93+1.05
βˆ’1.37 		1.334+0.017
βˆ’0.044 		636.13+11.70
βˆ’47.69 d 		2012 Direct imaging [46]
Ο„ Ceti g 1.75+0.25
βˆ’0.40 		0.133+0.001
βˆ’0.002 		20+0.02
βˆ’0.01 d 		2017 Radial velocity [47]
Ο„ Ceti h 1.83+0.68
βˆ’0.26 		0.243Β±0.003 49.41+0.08
βˆ’0.10 d 		2017 Radial velocity [48]
Ο„ Geminorum b 20.6 1.17 305.5Β±0.1 d 2004 Radial velocity [49]
Ο… Andromedae b 1.7+0.33
βˆ’0.24 		0.0594Β±0.0003 4.61711Β±0.000014 d 1996 Radial velocity [50]
Ο… Andromedae c 13.98+2.3
βˆ’5.3 		0.829Β±0.043 241.26Β±0.64 d 1999 Radial velocity [51]
Ο… Andromedae d 10.25+0.7
βˆ’3.3 		0.1061Β±0.0011 1.27646Β±0.57 d 1999 Radial velocity [52]
Ο… Leonis b 0.51+0.06
βˆ’0.26 		1.18+0.11
βˆ’0.32 		385.2+2.8
βˆ’1.3 d 		2021 Radial velocity [53]
ψ1 Aquarii b 3.2 0.7 181.4±0.1 d 2013 Radial velocity [54]
Ο‰ Serpentis b 1.7 1.q 277.02+0.52
βˆ’0.51 d 		2013 Radial velocity [55]

References

  1. ^ "The Extrasolar Planet Encyclopaedia β€” Alpha Arietis b". exoplanet.eu. Retrieved 11 September 2023.
  2. ^ "The Extrasolar Planet Encyclopaedia β€” Aldebaran b". exoplanet.eu. Retrieved 11 September 2023.
  3. ^ "The Extrasolar Planet Encyclopaedia β€” Beta Cancri b". exoplanet.eu. Retrieved 11 September 2023.
  4. ^ "The Extrasolar Planet Encyclopaedia β€” Beta Pictoris b". exoplanet.eu. Retrieved 11 September 2023.
  5. ^ "The Extrasolar Planet Encyclopaedia β€” Beta Pictoris c". exoplanet.eu. Retrieved 11 September 2023.
  6. ^ "The Extrasolar Planet Encyclopaedia β€” Beta Ursae Minoris b". exoplanet.eu. Retrieved 11 September 2023.
  7. ^ "The Extrasolar Planet Encyclopaedia β€” Gamma Cephei Ab". exoplanet.eu. Retrieved 11 September 2023.
  8. ^ "The Extrasolar Planet Encyclopaedia β€” Gamma1 Leonis b". exoplanet.eu. Retrieved 11 September 2023.
  9. ^ "The Extrasolar Planet Encyclopaedia β€” Gamma Librae b". exoplanet.eu. Retrieved 11 September 2023.
  10. ^ "The Extrasolar Planet Encyclopaedia β€” Gamma Librae c". exoplanet.eu. Retrieved 11 September 2023.
  11. ^ "The Extrasolar Planet Encyclopaedia β€” Gamma Piscium b". exoplanet.eu. Retrieved 11 September 2023.
  12. ^ "The Extrasolar Planet Encyclopaedia β€” Epsilon Coronae Borealis b". exoplanet.eu. Retrieved 11 September 2023.
  13. ^ "The Extrasolar Planet Encyclopaedia β€” Epsilon Eridani b". exoplanet.eu. Retrieved 11 September 2023.
  14. ^ "The Extrasolar Planet Encyclopaedia β€” Epsilon Indi Ab". exoplanet.eu. Retrieved 11 September 2023.
  15. ^ "The Extrasolar Planet Encyclopaedia β€” Epsilon Tauri b". exoplanet.eu. Retrieved 11 September 2023.
  16. ^ "The Extrasolar Planet Encyclopaedia β€” Iota Draconis b". exoplanet.eu. Retrieved 11 September 2023.
  17. ^ "The Extrasolar Planet Encyclopaedia β€” Iota Draconis c". exoplanet.eu. Retrieved 11 September 2023.
  18. ^ "The Extrasolar Planet Encyclopaedia β€” Kappa Andromedae b". exoplanet.eu. Retrieved 11 September 2023.
  19. ^ "The Extrasolar Planet Encyclopaedia β€” Kappa Coronae Borealis b". exoplanet.eu. Retrieved 11 September 2023.
  20. ^ "The Extrasolar Planet Encyclopaedia β€” Mu Arae b". exoplanet.eu. Retrieved 11 September 2023.
  21. ^ "The Extrasolar Planet Encyclopaedia β€” Mu Arae c". exoplanet.eu. Retrieved 11 September 2023.
  22. ^ "The Extrasolar Planet Encyclopaedia β€” Mu Arae d". exoplanet.eu. Retrieved 11 September 2023.
  23. ^ "The Extrasolar Planet Encyclopaedia β€” Mu Arae e". exoplanet.eu. Retrieved 11 September 2023.
  24. ^ "The Extrasolar Planet Encyclopaedia β€” Mu Leonis b". exoplanet.eu. Retrieved 11 September 2023.
  25. ^ "The Extrasolar Planet Encyclopaedia β€” Mu2 Scorpii b". exoplanet.eu. Retrieved 11 September 2023.
  26. ^ "The Extrasolar Planet Encyclopaedia β€” Nu Octantis Ab". exoplanet.eu. Retrieved 11 September 2023.
  27. ^ "The Extrasolar Planet Encyclopaedia β€” Nu Ophiuchi b". exoplanet.eu. Retrieved 11 September 2023.
  28. ^ "The Extrasolar Planet Encyclopaedia β€” Nu Ophiuchi c". exoplanet.eu. Retrieved 11 September 2023.
  29. ^ "The Extrasolar Planet Encyclopaedia β€” Xi Aquilae b". exoplanet.eu. Retrieved 11 September 2023.
  30. ^ "The Extrasolar Planet Encyclopaedia β€” Omicron Coronae Borealis b". exoplanet.eu. Retrieved 11 September 2023.
  31. ^ "The Extrasolar Planet Encyclopaedia β€” Omicron Ursae Majoris b". exoplanet.eu. Retrieved 11 September 2023.
  32. ^ "The Extrasolar Planet Encyclopaedia β€” Pi Mensae b". exoplanet.eu. Retrieved 11 September 2023.
  33. ^ "The Extrasolar Planet Encyclopaedia β€” Pi Mensae c". exoplanet.eu. Retrieved 11 September 2023.
  34. ^ "The Extrasolar Planet Encyclopaedia β€” Pi Mensae d". exoplanet.eu. Retrieved 11 September 2023.
  35. ^ "The Extrasolar Planet Encyclopaedia β€” Rho1 Cancri b". exoplanet.eu. Retrieved 11 September 2023.
  36. ^ "The Extrasolar Planet Encyclopaedia β€” Rho1 Cancri c". exoplanet.eu. Retrieved 11 September 2023.
  37. ^ "The Extrasolar Planet Encyclopaedia β€” Rho1 Cancri d". exoplanet.eu. Retrieved 11 September 2023.
  38. ^ "The Extrasolar Planet Encyclopaedia β€” Rho1 Cancri e". exoplanet.eu. Retrieved 11 September 2023.
  39. ^ "The Extrasolar Planet Encyclopaedia β€” Rho1 Cancri f". exoplanet.eu. Retrieved 11 September 2023.
  40. ^ "The Extrasolar Planet Encyclopaedia β€” Rho Coronae Borealis b". exoplanet.eu. Retrieved 11 September 2023.
  41. ^ "The Extrasolar Planet Encyclopaedia β€” Rho Coronae Borealis c". exoplanet.eu. Retrieved 11 September 2023.
  42. ^ "The Extrasolar Planet Encyclopaedia β€” Rho Coronae Borealis d". exoplanet.eu. Retrieved 11 September 2023.
  43. ^ "The Extrasolar Planet Encyclopaedia β€” Rho Coronae Borealis e". exoplanet.eu. Retrieved 11 September 2023.
  44. ^ "The Extrasolar Planet Encyclopaedia β€” Tau BoΓΆtis b". exoplanet.eu. Retrieved 11 September 2023.
  45. ^ "The Extrasolar Planet Encyclopaedia β€” Tau Ceti e". exoplanet.eu. Retrieved 11 September 2023.
  46. ^ "The Extrasolar Planet Encyclopaedia β€” Tau Ceti f". exoplanet.eu. Retrieved 11 September 2023.
  47. ^ "The Extrasolar Planet Encyclopaedia β€” Tau Ceti g". exoplanet.eu. Retrieved 11 September 2023.
  48. ^ "The Extrasolar Planet Encyclopaedia β€” Tau Ceti h". exoplanet.eu. Retrieved 11 September 2023.
  49. ^ "The Extrasolar Planet Encyclopaedia β€” Tau Geminorum b". exoplanet.eu. Retrieved 11 September 2023.
  50. ^ "The Extrasolar Planet Encyclopaedia β€” Upsilon Andromedae b". exoplanet.eu. Retrieved 11 September 2023.
  51. ^ "The Extrasolar Planet Encyclopaedia β€” Upsilon Andromedae c". exoplanet.eu. Retrieved 11 September 2023.
  52. ^ "The Extrasolar Planet Encyclopaedia β€” Upsilon Andromedae d". exoplanet.eu. Retrieved 11 September 2023.
  53. ^ "The Extrasolar Planet Encyclopaedia β€” Upsilon Leonis b". exoplanet.eu. Retrieved 11 September 2023.
  54. ^ "The Extrasolar Planet Encyclopaedia β€” Psi1 Aquarii b". exoplanet.eu. Retrieved 11 September 2023.
  55. ^ "The Extrasolar Planet Encyclopaedia β€” Omega Serpentis b". exoplanet.eu. Retrieved 11 September 2023.

CoRoT-7/Kepler-90

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