Magnetic interaction of super-Earths with their host star and planet composition
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2010.
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| Format: | Thesis |
| Language: | eng |
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Massachusetts Institute of Technology
2011
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| Online Access: | http://hdl.handle.net/1721.1/61258 |
| _version_ | 1826188753033494528 |
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| author | Piso, Ana-Maria (Ana-Maria Adriana) |
| author2 | Paola Rebusco and Sara Seager. |
| author_facet | Paola Rebusco and Sara Seager. Piso, Ana-Maria (Ana-Maria Adriana) |
| author_sort | Piso, Ana-Maria (Ana-Maria Adriana) |
| collection | MIT |
| description | Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2010. |
| first_indexed | 2024-09-23T08:04:10Z |
| format | Thesis |
| id | mit-1721.1/61258 |
| institution | Massachusetts Institute of Technology |
| language | eng |
| last_indexed | 2024-09-23T08:04:10Z |
| publishDate | 2011 |
| publisher | Massachusetts Institute of Technology |
| record_format | dspace |
| spelling | mit-1721.1/612582022-01-13T07:54:41Z Magnetic interaction of super-Earths with their host star and planet composition Piso, Ana-Maria (Ana-Maria Adriana) Paola Rebusco and Sara Seager. Massachusetts Institute of Technology. Dept. of Physics. Massachusetts Institute of Technology. Department of Physics Physics. Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2010. Cataloged from PDF version of thesis. Includes bibliographical references (p. 75-78). We study the magnetic field and the planet-star interactions of super Earths, extrasolar planets with masses between 1 and 10 times the mass of the Earth. We first present a model of the magnetic field of a super Earth, the dynamo model. We then list and explain several mechanisms through which magnetic energy can be released, as well as various ways through which the power dissipated can be observed. We apply our model to two recently discovered super Earths, CoRoT 7-b and GJ 1214 b. We find that emission from CoRoT 7-b is very low and thus unlikely to be observable, while emission from GJ 1214 b may be detectable with current instruments and its measurement can provide information regarding the internal composition of the planet. Further on, we discuss some special cases for detection, such as M and Ap type stars. We conclude our thesis with a generalization of our results and guidelines for future developments. by Ana-Maria Piso. S.B. 2011-02-23T14:37:47Z 2011-02-23T14:37:47Z 2010 2010 Thesis http://hdl.handle.net/1721.1/61258 701908664 eng M.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission. http://dspace.mit.edu/handle/1721.1/7582 78 p. application/pdf Massachusetts Institute of Technology |
| spellingShingle | Physics. Piso, Ana-Maria (Ana-Maria Adriana) Magnetic interaction of super-Earths with their host star and planet composition |
| title | Magnetic interaction of super-Earths with their host star and planet composition |
| title_full | Magnetic interaction of super-Earths with their host star and planet composition |
| title_fullStr | Magnetic interaction of super-Earths with their host star and planet composition |
| title_full_unstemmed | Magnetic interaction of super-Earths with their host star and planet composition |
| title_short | Magnetic interaction of super-Earths with their host star and planet composition |
| title_sort | magnetic interaction of super earths with their host star and planet composition |
| topic | Physics. |
| url | http://hdl.handle.net/1721.1/61258 |
| work_keys_str_mv | AT pisoanamariaanamariaadriana magneticinteractionofsuperearthswiththeirhoststarandplanetcomposition |