File:Nearest terrestrial habitable exoplanets.png
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Summary
[edit]DescriptionNearest terrestrial habitable exoplanets.png |
English: Nearest stars with terrestrial ("rocky") exoplanets candidates at a distance of up to 50 light-years from the Solar System.
- at least one of terrestrial exoplanets in the system lying inside the star's habitable zone (names of host stars also shown) - terrestrial exoplanets, but outside the habitable zone Positions of the dots represent a distance of the host star from the Solar System and a right ascension of the host star. They don't represent distances between host stars. Right ascension: clockwise, from the upper point of the diagram. Note: There is still some uncertainty among scientists about terrestrial composition or habitability of most of exoplanets. Sources listed below confirm the possibility of terrestrial composition and habitability. Sources: [1] [2] [3] [4] [5] [6] [7] [8] [9] [10] [11] [12] [13] [14] |
Date | |
Source | Own work |
Author | Zhitelew |
References
[edit]- ↑ https://arxiv.org/abs/1403.0430
- ↑ http://phys.org/news/2014-06-astronomers-ancient-worlds-galaxy-door.html
- ↑ Eugenio J. Rivera, Gregory Laughlin, R. Paul Butler, Steven S. Vogt, Nader Haghighipour, Stefano Meschiari (2010). \"The Lick-Carnegie Exoplanet Survey: A Uranus-mass Fourth Planet for GJ 876 in an Extrasolar Laplace Configuration\".
- ↑ http://www.hpcf.upr.edu/~abel/phl/tuomi/hec_orbit_GJ_682_b.png
- ↑ Schneider, Jean, "Star: HD 20794", Extrasolar Planets Encyclopaedia (Paris Observatory), retrieved 2011-12-05
- ↑ Vogt, S. S.; et al. (2010). \"The Lick-Carnegie Exoplanet Survey: A 3.1 M_Earth Planet in the Habitable Zone of the Nearby M3V Star Gliese 581
- ↑ http://phl.upr.edu/projects/habitable-exoplanets-catalog
- ↑ Vogt, Steven (2009). \"A Super-Earth and two Neptunes Orbiting the Nearby Sun-like star 61 Virginis
- ↑ Kaltenegger, L.; Udry, S.; Pepe, F. (2011). A Habitable Planet around HD 85512?
- ↑ Rebekah et al.; Fabrycky (2010-05-21). \"Radial velocity planets de-aliased. A new, short period for Super-Earth 55 Cnc e\". The Astrophysical Journal 722: 937–953
- ↑ M. Mayor, S. Udry, C. Lovis, F. Pepe, D. Queloz, W. Benz, J.-L. Bertaux, F. Bouchy, C. Mordasini, D. Segransan (2009). \"The HARPS search for southern extra-solar planets. XIII. A planetary system with 3 Super-Earths (4.2, 6.9, & 9.2 Earth masses)\". Astronomy and Astrophysics 493 (2): 639–644
- ↑ M. Mayor, S. Udry, C. Lovis, F. Pepe, D. Queloz, W. Benz, J.-L. Bertaux, F. Bouchy, C. Mordasini, D. Segransan (2009). \"The HARPS search for southern extra-solar planets. XIII. A planetary system with 3 Super-Earths (4.2, 6.9, & 9.2 Earth masses)\". Astronomy and Astrophysics 493 (2): 639–644.
- ↑ Bonfils; Delfosse; Udry; Forveille; Mayor; Perrier; Bouchy; Gillon et al. (2011). "The HARPS search for southern extra-solar planets XXXI. The M-dwarf sample". arXiv:1111.5019 [astro-ph.EP
- ↑ http://phl.upr.edu/press-releases/gliese832
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Horizontal resolution | 49.61 dpc |
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File change date and time | 10:40, 1 July 2014 |