List of super-earths

from Wikipedia, the free encyclopedia

Listed here are the previously known super-earths , i.e. extrasolar terrestrial planets .

In most of these planets, the earth-like structure has not yet been proven beyond doubt (see main article ) . Definitely proven rock planets are shown in bold .

Super-earths

Super-earths discovered so far:

In the future, the number of known super-earths could increase dramatically if many of the Kepler Space Telescope's planet candidates are confirmed. Of the 1235 candidates discovered by early February 2011, 288 are super-earths.

Surname discovery star Distance ( Lj ) Mass (1) ( M E ) Radius (2) ( km ) Orbital time ( d ) eccentricity
earth - Sun - 1 6,370 365.256 0.0167
PSR 1257 + 12 c 1991 PSR 1257 + 12 978.6 4.13 ± 0.19 9,400 66.5419 0.0186
PSR 1257 + 12 d 1991 3.81 ± 0.19 9,200 98.2114 0.0252
Gliese 876 d 2005 Peter 876 15.4 > 6.83 ± 0.40 10,000 1.93778 0.207 ± 0.055
OGLE-2005-BLG-390Lb 2006 OGLE-2005-BLG-390L ≈21,200 > 5.40 - ≈3,500 -
HD 69830 b 2006 HD 69830 41.1 > 10.49 12,000 8.667 0.1 ± 0.04
Gliese 581 c 2007 Jean 581 20.4 > 5.36 9,500 12.9292 0.17 ± 0.07
Gliese 581 e 2009 > 1.94 - 3.14942
MOA-2007-BLG-192-Lb 2008 MOA-2007-BLG-192-L 1 ≈3,000 3.2 +4.9 -1.6 - - -
HD 40307 b 2008 HD 40307 41.8 > 4.20 - 4.3115 0
HD 40307 c 2008 > 6.87 - 9.62 ± 0.02 0
HD 40307 d 2008 > 9.16 - 20.46 ± 0.01 0
HD 181433 b 2008 HD 181433 85.3 > 7.57 - 9.3743 0.396 ± 0.06
CoRoT-7 b 2009 CoRoT-7 2 456.7 4.8 ± 0.8 11,000 0.853585 0
CoRoT-7 c 2009 8.4 ± 0.9 - 3,698 0
HD 7924 b 2009 HD 7924 54.8 > 9.26 - 5.3978 0.17 ± 0.16
61 Vir b 2009 61 Vir 27.8 > 5.1 ± 0.6 - 4.215 0.12 ± 0.11
HD 1461 b 2009 HD 1461 3 76.3 > 7.6 ± 1.2 - 5.7727 0.14 ± 0.19
FY 1214 b 2009 FY 1214 42.4 6.55 ± 0.98 17,000 1.58040 <0.27
Kepler-10 b 2011 Kepler-10 564.2 4.56 +1.17 -1.29 9,000 0.83749 0
Kepler-11 b 2011 Kepler-11 ≈2,000 4.3 +2.2 -2.0 12,500 10.30375 0
Kepler-11 d 2011 6.1 +3.1 -1.7 21,800 22.68719 0
Kepler-11 e 2011 8.4 +2.5 -1.9 28,800 31,9959 0
Kepler-11 f 2011 2.3 +2.2 -1.2 16,600 46.68876 0
Gliese 667Cc 2011/12 Gliese 667C ≈22 > 4.5 ≈28.15

Remarks

(1)Due to the neglected and often unknown inclination, the known mass is mostly only the lower limit of the possible planetary mass, represented by ">".
(2)The radius information is an estimate - all other astrometric and physical information is measurement-based approximate values

Footnotes

1The latest findings indicate that the mass of the parent star is significantly higher and that it is not a brown but a red dwarf, which results in a newly determined mass of only 1.4 Earth masses for the exoplanet . Should this be confirmed, there would be no system around a brown dwarf as yet.
2another exoplanet CoRoT-7d unconfirmed; if confirmed, different values ​​for CoRoT-7 b and c
3Exoplanets HD 1461 c and d unconfirmed; given values ​​correspond to the 1-planet scenario

See also

Web links

Individual evidence

  1. Articles published and reviewed by active institutions and leading journals in astronomy and astrophysics :