On the Unexplained Density of Exoplanet TrES-4: Difference between revisions
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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 /> | ||
[[Category:Scientific Paper|unexplained density exoplanet tres-]] | |||
[[Category:Gravity]] | [[Category:Gravity]] | ||
[[Category:Cosmology]] | [[Category:Cosmology]] | ||
Revision as of 13:51, 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.