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  2. Orbit of Mars - Wikipedia

    en.wikipedia.org/wiki/Orbit_of_Mars

    Extra-close oppositions of Mars happen every 15 to 17 years, when we pass between Mars and the Sun around the time of its perihelion (closest point to the Sun in orbit). The minimum distance between Earth and Mars has been declining over the years, and in 2003 the minimum distance was 55.76 million km, nearer than any such encounter in almost ...

  3. Apsis - Wikipedia

    en.wikipedia.org/wiki/Apsis

    The apsides refer to the farthest (2) and nearest (3) points reached by an orbiting planetary body (2 and 3) with respect to a primary, or host, body (1). An apsis (from Ancient Greek ἁψίς (hapsís) 'arch, vault'; pl. apsides / ˈ æ p s ɪ ˌ d iː z / AP-sih-deez) [1] [2] is the farthest or nearest point in the orbit of a planetary body about its primary body.

  4. Astronomy on Mars - Wikipedia

    en.wikipedia.org/wiki/Astronomy_on_Mars

    On both Earth and Mars, these two precessions are in opposite directions, and therefore add, to make the precession cycle between the tropical and anomalistic years 21,000 years on Earth and 29,700 Martian years (55,900 Earth years) on Mars. As on Earth, the period of rotation of Mars (the length of its day) is slowing down.

  5. File:Mars earth orbit.svg - Wikipedia

    en.wikipedia.org/wiki/File:Mars_earth_orbit.svg

    English: Orbits of Mars and Earth seen from the north. Also shows lengths of seasons, equinoxes, solstices, perihelion and aphelion. Also shows lengths of seasons, equinoxes, solstices, perihelion and aphelion.

  6. Kepler's laws of planetary motion - Wikipedia

    en.wikipedia.org/wiki/Kepler's_laws_of_planetary...

    Log-log plot of period T vs semi-major axis a (average of aphelion and perihelion) ... Earth 1 365.2564 7.496 Mars 1.52366 686.9796 7.495 Jupiter 5.20336 4332.8201

  7. Mars - Wikipedia

    en.wikipedia.org/wiki/Mars

    At their furthest Mars and Earth can be as far as 401 million km (249 million mi) apart. [191] Mars comes into opposition from Earth every 2.1 years. The planets come into opposition near Mars's perihelion in 2003, 2018 and 2035, with the 2020 and 2033 events being particularly close to perihelic opposition. [192] [193] [194]

  8. Earth's orbit - Wikipedia

    en.wikipedia.org/wiki/Earth's_orbit

    The six Earth images are positions along the orbital ellipse, which are sequentially the perihelion (periapsis—nearest point to the Sun) on anywhere from January 2 to January 5, the point of March equinox on March 19, 20, or 21, the point of June solstice on June 20, 21, or 22, the aphelion (apoapsis—the farthest point from the Sun) on ...

  9. Martian dichotomy - Wikipedia

    en.wikipedia.org/wiki/Martian_dichotomy

    The spin axis of Mars, as with many bodies, precesses over millions of years. At present, the solstices nearly coincide with Mars's aphelion and perihelion. This results in one hemisphere, the Southern, receiving more sunlight in summer and less in winter, and thus more extreme temperatures, than the Northern.