Rake ootcome fer
Mak the page "Orbital+period" on this wiki! See the rake ootcome fand as weel.
frae the planet's solar day, whilk includes an extra fractional rotation needit tae accommodate the portion o the planet's orbital period in ane day.... |
solutions tae the orbital period. Uisin a 1950 epoch, Sedna haes a 12,100-year period, but uisin a 2010 epoch Sedna haes an 11,800-year period. For objects... |
closest tae the Sun o the aicht planets in the Solar Seestem, wi an orbital period o aboot 88 Yird days. Seen frae the Yird, it appears tae muive aroond... |
time based on tha orbital period o tha Yird movin aroond tha Sun. Fur an observer at is oan tha Yird, thes corresponds tae tha period it taes tha sun tae... |
lairge asteroid frae the asteroid belt. "AstDyS-2 Astraea Synthetic Proper Orbital Elements". Department of Mathematics, University of Pisa, Italy. Retrieved... |
Hygiea". Retrieved 7 September 2008. "AstDyS-2 Hygiea Synthetic Proper Orbital Elements". Department of Mathematics, University of Pisa, Italy. Retrieved... |
hauf a percent o the mass o the belt. "AstDyS-2 Hebe Synthetic Proper Orbital Elements". Department of Mathematics, University of Pisa, Italy. Retrieved... |
an Jupiter. Oxford English Dictionary "AstDyS-2 Iris Synthetic Proper Orbital Elements". Department of Mathematics, University of Pisa, Italy. Retrieved... |
September 2008). Retrieved 10 November 2008. "AstDyS-2 Metis Synthetic Proper Orbital Elements". Department of Mathematics, University of Pisa, Italy. Retrieved... |
Julie 2008. Retrieved 1 November 2008. "AstDyS-2 Juno Synthetic Proper Orbital Elements". Department of Mathematics, University of Pisa, Italy. Retrieved... |
Jacobson, R.A. (2009) SAT317 (17 December 2009). "Planetary Satellite Mean Orbital Parameters". JPL/NASA. Retrieved 15 Januar 2011. Roatsch, T.; Jaumann,... |
Unknown parameter |deadurl= ignored (help) "AstDyS-2 Ceres Synthetic Proper Orbital Elements". Department of Mathematics, University of Pisa, Italy. Archived... |
Browser: 4 Vesta". Retrieved 1 Juin 2008. "AstDyS-2 Vesta Synthetic Proper Orbital Elements". Department of Mathematics, University of Pisa, Italy. Retrieved... |
Retrieved 17 December 2009. Horizons output. "Barycentric Osculating Orbital Elements for Comet C/1995 O1 (Hale-Bopp)". Retrieved 31 Januar 2011. (Solution... |
an aither a main sequence, sub-giant, or reid giant starn. Whan the orbital period faws in the range o several days tae ane day, the white dwarf is close... |
Pallas". Retrieved 12 September 2009. "AstDyS-2 Pallas Synthetic Proper Orbital Elements". Department of Mathematics, University of Pisa, Italy. Retrieved... |
Muin's mean sidereal period (fixed starn tae fixed starn) is 27.321661 days (27 d 07 o 43 meen 11.5 s), an its mean tropical orbital period (frae equinox tae... |
418 km (260 mi) AMSL Orbital inclination 51.65 degrees Average speed 7.66 kilometres per second (27,600 km/h; 17,100 mph) Orbital period 92.87 minutes Orbit... |
Semi-major axis 349.166 Gm (2.334 AU) Eccentricity 0.221 Orbital period 1302.439 d (3.57 a) Average orbital speed 19.50 km/s Mean anomaly 80.591° Inclination... |
751x751x715 – Wolfram-Alpha". A. N. Heinze and Daniel deLahunta, The rotation period and light-curve amplitude of Kuiper belt dwarf planet 136472 Makemake (2005... |