As the number of detected extrasolar planets increases, exoplanet databases become a valuable resource, confirming some details about planetary formation but also challenging our theories with new, unexpected properties. Key Words: Exoplanets—Gravity—Planetary habitability and biosignatures. Astrobiology 16, 325–327.
Get full access to this article
View all access options for this article.
References
1.
BasriG., BoruckiW.J., and KochD. (2005) The Kepler mission: a wide-field transit search for terrestrial planets. New Astronomy Reviews, 49:478–485.
2.
EO. (2016) The Exoplanet Orbit Database. Available online at http://exoplanets.org
3.
EPE. (2016) The Extrasolar Planets Encyclopaedia. Available online at http://www.exoplanet.eu
4.
EspinozaN., BrahmR., JordánA., JenkinsJ.S., RojasF., JofréP., MädlerT., RabusM., ChanaméJ., PantojaB., and SotoM.G. (2016) A Neptune-sized exoplanet consistent with a pure rock composition. arXiv:1601.07608.
5.
HowardA.W. (2013) Observed properties of extrasolar planets. Science, 340:572–576.
6.
JacobsonR.A. (2009) The orbits of the neptunian satellites and the orientation of the pole of Neptune. Astron J, 137:4322–4329.
7.
MayorM. and QuelozD. (1995) A Jupiter-mass companion to a solar-type star. Nature, 378:355–359.
8.
MordasiniC., MollièreP., DittkristK.M., JinS., and AlibertY. (2015) Global models of planet formation and evolution. International Journal of Astrobiology, 14:201–232.
9.
NEA. (2016) NASA Exoplanet Archive. Available online at http://exoplanetarchive.ipac.caltech.edu
10.
OEC. (2016) The Open Exoplanet Catalogue. Available online at http://www.openexoplanetcatalogue.com
11.
RaymondS.N., BarnesR., and MandellA.M. (2008) Observable consequences of planet formation models in systems with close-in terrestrial planets. Mon Not R Astron Soc, 384:663–674.
12.
RogersL.A. (2015) Most 1.6 Earth-radius planets are not rocky. Astrophys J, 801, doi:10.1088/0004-637X/801/1/41.
13.
RosenblattF. (1971) A two-color photometric method for detection of extra-solar planetary systems. Icarus, 14:71–93.
14.
SeagerS., KuchnerM., Hier-MajumderC.A., and MilitzerB. (2007) Mass-radius relationships for solid exoplanets. Astrophys J, 669:1279–1297.
15.
SouthworthJ., WheatleyP.J., and SamsG. (2007) A method for the direct determination of the surface gravities of transiting extrasolar planets. Mon Not R Astron Soc Lett, 379:L11–L15.
16.
SpiegelD.S., FortneyJ.J., and SotinC. (2014) Structure of exoplanets. Proc Natl Acad Sci USA, 111:12622–12627.