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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. Mars sol - Wikipedia

    en.wikipedia.org/wiki/Mars_sol

    Sol (borrowed from the Latin word for sun) is a solar day on Mars; that is, a Mars-day. A sol is the apparent interval between two successive returns of the Sun to the same meridian (sundial time) as seen by an observer on Mars. It is one of several units for timekeeping on Mars. A sol is slightly longer than an Earth day.

  4. Mars - Wikipedia

    en.wikipedia.org/wiki/Mars

    The average time between the successive oppositions of Mars, its synodic period, is 780 days; but the number of days between successive oppositions can range from 764 to 812. [189] The distance at close approach varies between about 54 and 103 million km (34 and 64 million mi) due to the planets' elliptical orbits, which causes comparable ...

  5. Astronomy on Mars - Wikipedia

    en.wikipedia.org/wiki/Astronomy_on_Mars

    An illustration of what Mars may have looked like during an ice age about 400,000 years ago caused by a large axial tilt. As on Earth, the effect of precession causes the north and south celestial poles to move in a very large circle, but on Mars the cycle is 95,500 Martian years (179,600 Earth years) [24] rather than 26,000 years as on Earth.

  6. Transit of Earth from Mars - Wikipedia

    en.wikipedia.org/wiki/Transit_of_Earth_from_Mars

    Earth and Moon transiting the Sun in 2084, as seen from Mars. Image created using SpaceEngine Earth and Moon from Mars, as photographed by the Mars Global Surveyor. A transit of Earth across the Sun as seen from Mars takes place when the planet Earth passes directly between the Sun and Mars, obscuring a small part of the Sun's disc for an observer on Mars.

  7. Mars Year 1 - Wikipedia

    en.wikipedia.org/wiki/Mars_Year_1

    Mars Years have no officially adopted month systems. Scientists generally use two sub-units of the Mars Year: the Solar longitude (L s) system: 360 degrees per Mars Year that represent the position of Mars in its orbit around the Sun, or; the Sol system: 668 sols per Mars Year. This system consists of uniform time units. However, Mars Year sols ...

  8. The Sun in Capricorn Opposite Mars Retrograde Is All About ...

    www.aol.com/sun-capricorn-opposite-mars...

    The Sun in Capricorn Opposite Mars Retrograde Is All About Ambition, and These 4 Signs Are About to Have Their Work-Life Balance Rocked Valerie Mesa January 15, 2025 at 10:00 AM

  9. Vicarious Hypothesis - Wikipedia

    en.wikipedia.org/wiki/Vicarious_Hypothesis

    While the heliocentric longitudes of this model proved to be accurate, distances from the Sun to Mars, or latitudes of Mars, challenged the model. In his book, Astronomia Nova , Kepler determined that the eccentricity of the Sun, based on latitudinal oppositions, should be between a range of 8,000 and 9,943, conflicting with the eccentricity of ...