The Possible Interrelation of Trans - Neptunian Objects and Long - Period Comets with the High-Precision Orbits
Ayyub Guliyev,
Shaig Nabiyev
Issue:
Volume 2, Issue 4, July 2014
Pages:
38-41
Received:
31 July 2014
Accepted:
15 August 2014
Published:
30 August 2014
Abstract: The question on the relationship of long-period comets (LPCs) with trans-Neptunian objects (ТNОs) having the diameter more than 200 km is investigated. We analyze the distribution values of minimum orbit intersection distances (МОID) for 91 TNOs and 495 long-period comets (LPCs) with known initial orbits. The parameter t – distribution characterizing the level of redundancy МОID for each selected planetary body is prefaced. In the case when МОIDs values are less than 1 AU, 14 values of t have significance, greater than 0.95, and for the case MOIDs less than 0.5 AU, 6 values of t have significance, more than 0.95, and the ratio of t makes 56:35 and 50:41, accordingly. A reliable correlation no matter it is weak, between values t and I (inclination) is found out. The obtained these results indicate the assumption of possible relation of long-period comets with TNOs.
Abstract: The question on the relationship of long-period comets (LPCs) with trans-Neptunian objects (ТNОs) having the diameter more than 200 km is investigated. We analyze the distribution values of minimum orbit intersection distances (МОID) for 91 TNOs and 495 long-period comets (LPCs) with known initial orbits. The parameter t – distribution characterizi...
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Variation of Gravitational Constant w. r. t. the Spinning Velocity of Super Dense Stars in Very Strong Gravitational Field
Md Shams Nadeem,
Dipo Mahto,
Kumari Vineeta,
Krishna Murari Singh
Issue:
Volume 2, Issue 4, July 2014
Pages:
42-46
Received:
13 August 2014
Accepted:
30 August 2014
Published:
20 September 2014
Abstract: Mahto et al. have derived the formula for the variation of the gravitational constant given by G^'=G/√(1-v^2/c^2 ) in very strong gravitational field of the compact bodies like super massive black holes and neutron stars (2013). In this paper, we have extended this work to show that the variation of gravitational constant in the strong gravitational field with respect to the spinning velocity of super dense stars is directly proportional to its spinning velocity.
Abstract: Mahto et al. have derived the formula for the variation of the gravitational constant given by G^'=G/√(1-v^2/c^2 ) in very strong gravitational field of the compact bodies like super massive black holes and neutron stars (2013). In this paper, we have extended this work to show that the variation of gravitational constant in the strong gravitationa...
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