Difference between revisions of "On the Unexplained Density of Exoplanet TrES-4"
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==Abstract== | ==Abstract== | ||
− | The exoplanet TrES-4 has been discovered in 2007. Its density is 0.24 gr/cm?? and its diameter is 1.7 times that of Jupiter. The orbital radius is 7.3.109 m and the orbital period is 3.5 days about a star which has a mass of 1.2 M??. It is not known why such low-density planets can exist. Low-density planets should quickly become more dense, due to gravitation.<br />[[Category:Scientific Paper]] | + | The exoplanet TrES-4 has been discovered in 2007. Its density is 0.24 gr/cm?? and its diameter is 1.7 times that of Jupiter. The orbital radius is 7.3.109 m and the orbital period is 3.5 days about a star which has a mass of 1.2 M??. It is not known why such low-density planets can exist. Low-density planets should quickly become more dense, due to gravitation.<br /> |
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+ | [[Category:Scientific Paper|unexplained density exoplanet tres-]] | ||
[[Category:Gravity]] | [[Category:Gravity]] | ||
[[Category:Cosmology]] | [[Category:Cosmology]] |
Revision as of 10:51, 1 January 2017
Scientific Paper | |
---|---|
Title | On the Unexplained Density of Exoplanet TrES-4 |
Read in full | Link to paper |
Author(s) | Thierry De Mees |
Keywords | TrES-4, exoplanet, gravitation, gravitomagnetism, rotary star, gyrotation |
Published | 2007 |
Journal | General Science Journal |
No. of pages | 2 |
Read the full paper here
Abstract
The exoplanet TrES-4 has been discovered in 2007. Its density is 0.24 gr/cm?? and its diameter is 1.7 times that of Jupiter. The orbital radius is 7.3.109 m and the orbital period is 3.5 days about a star which has a mass of 1.2 M??. It is not known why such low-density planets can exist. Low-density planets should quickly become more dense, due to gravitation.