Rotation period: 1.026 solar days Revolution period: 686.98 solar days Obliquity: 25° Orbit (inclination degree): 1.85° Orbit eccentricity: .0.093° Max. surface temperature: 310° K Min. surface temperature: 150° K Visual geometric albedo: 0.15 Highest point on surface: Olympus Mons Atmospheri...
Mars and Earth are quite different. Compared to Earth, a year on Mars lasts almost twice as long – 686.98 Earth days. This is due to the fact that Mars is significantly farther from the Sun and its orbital period (the time it takes to orbit the Sun) is significantly greater than that...
"Let nothing dissuade your Quest for Knowledge. Let none slow your pursuit and acquisition of holy technology. Let no one stand between you and the procurement of that which is rightfully the Machine God's due." —Thusdorius Knoch, Invictus Acquisitor Ma
Jupiter has different rotation periods per latitude, so devising a calendar system for the gas giant would pose a whole new set of challenges compared to terrestrial planets like Mars. ©NASA, ESA, STScI, A. Simon (Goddard Space Flight Center), M.H. Wong (University of California, Berkele...
Synodic period 779.96 day2.135 Julian years Average orbital speed 24.077 km/s Inclination 1.850掳5.65掳 to Sun's Equator Longitude of ascending node 49.562掳 Argument of perihelion 286.537掳 Satellites 2 Physical characteristics Equatorial radius 3 396.2 卤 0.1 km[a][2]0.533 Earths Polar radius 3 ...
Figure 1a,b shows the diurnal cycle of retrieved fluxes and surface temperature, respectively. Figure 1d shows the diurnal evolution of measured albedo on the sols with the highest (sol 125) and lowest (sol 209) values of the studied period. On both sols, the minimum value is reached near...
distancefromthesunTheaveragespeedoforbitingthesundiameterTheinclinationofrotationaxisOrbitalperiodThelengthofadayEquatorialsurfacegravityaveragetemperatureatmosphere 15millionkm29.772km/sec12755.661km23.5°365.25days23hoursand56minutes9.8m/sec213.88℃N2(78%)、O2(21%)、227.94millionkm23.335km/sec6791....
the crew capsule would maneuver itself away from the upper stage while inducing an end-over-end spin in the system. Eventual rotation speed depends on the tether length, difference in mass between the crew capsule and the upper stage, and the desired gravity field. The system would continue ...
On the other hand, if the tidal bump trails behind a moon, then that moon is slowed down and drops lower as a result. Phobos’ orbital period is about 8 hours (it’s already very low), and Mars’ day (a “sol“) is about as long as ours, so the bump Phobos creates necessari...
The Emirates Mars Mission (EMM) was launched to Mars in the summer of 2020, and is the first interplanetary spacecraft mission undertaken by the United Arab Emirates (UAE). The mission has multiple programmatic and scientific objectives, including the return of scientifically useful information about...