ECCENTRICITY FROM TRANSIT PHOTOMETRY: SMALL PLANETS IN KEPLER MULTI-PLANET SYSTEMS HAVE LOW ECCENTRICITIES
Solar system planets move on almost circular orbits. In strong contrast, many massive gas giant exoplanets travel on highly elliptical orbits, whereas the shape of the orbits of smaller, more terrestrial, exoplanets remained largely elusive. Knowing the eccentricity distribution in systems of small...
| मुख्य लेखकों: | , |
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| अन्य लेखक: | |
| स्वरूप: | लेख |
| भाषा: | en_US |
| प्रकाशित: |
IOP Publishing
2015
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| ऑनलाइन पहुंच: | http://hdl.handle.net/1721.1/99914 |