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]]
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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:Gravity]]
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[[Category:Scientific Paper|unexplained density exoplanet tres-]]
[[Category:Cosmology]]
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[[Category:Gravity|unexplained density exoplanet tres-]]
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[[Category:Cosmology|unexplained density exoplanet tres-]]

Latest revision as of 19:48, 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.