semimajor axis การใช้

• Like HD 47536 b, mass and semimajor axis are not exactly known.
• The two stars are separated by a semimajor axis of 7.61 AUs.
• Then with semimajor axis " a ", the eccentricity is given by
• The boundary for the semimajor axis is surprisingly sharp for the prograde satellites.
• The semimajor axis is 8-9 AU and its orbital period is 17 21 years.
• Geodesists, by convention, use the semimajor axis and flattening.
• They orbit around each other every 11.6 years with a semimajor axis of 0.4 arcseconds.
• However, it does have a semimajor axis near that of Uranus, making it a Uranus co-orbital.
• The secondary star B orbits A at only 9.8 times the semimajor axis of A's planet.
• However, as the semimajor axis of the Moon's orbit continues to increase, this stabilizing effect will diminish.
• The two are gravitationally bound and separated at 310 AU . The binary semimajor axis is 390 AU.
• Once phasing orbit period is determined, the phasing orbit semimajor axis can be derived from the period formula:
• So this planet will need couple more years of observations to better constrain the period and semimajor axis.
• It shows a noticeable amount of flattening, with an aspect ratio of between its semimajor axis and semiminor axis.
• The value for the semimajor axis ( a ) of the WGS 72 Ellipsoid is 6 378 135 meters.
• Semimajor axis is 3.84399E8 m.
• The semimajor axis of this 3.68 Jupiter mass planet is 0.97 astronomical units, taking approximately 326 days to revolve.
• The orbital period is 572 days and orbits at a semimajor axis of 1.35 eccentric orbits of any known planets.
• The semimajor axis would be 5.32 AU with an orbital period of 4100 ?7300 days ( 11 years ).
• The orbital semimajor axis is only 0.13 eccentric than the orbit of any of the major planets of our solar system.