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  2. Geology of solar terrestrial planets - Wikipedia

    en.wikipedia.org/wiki/Geology_of_solar...

    Terrestrial planets are substantially different from the giant planets, which might not have solid surfaces and are composed mostly of some combination of hydrogen, helium, and water existing in various physical states. Terrestrial planets have a compact, rocky surfaces, and Venus, Earth, and Mars each also has an atmosphere. Their size, radius ...

  3. Mars - Wikipedia

    en.wikipedia.org/wiki/Mars

    At one point, 1.35 million Earth years ago, Mars had an eccentricity of roughly 0.002, much less than that of Earth today. [188] Mars's cycle of eccentricity is 96,000 Earth years compared to Earth's cycle of 100,000 years. [189] Mars has its closest approach to Earth in a synodic period of 779.94 days. It should not be confused with Mars ...

  4. Terrestrial planet - Wikipedia

    en.wikipedia.org/wiki/Terrestrial_planet

    A terrestrial planet, telluric planet, or rocky planet, is a planet that is composed primarily of silicate, rocks or metals.Within the Solar System, the terrestrial planets accepted by the IAU are the inner planets closest to the Sun: Mercury, Venus, Earth and Mars.

  5. Geology of Mars - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Mars

    If placed on Earth, Valles Marineris would span the width of North America. [36] In places, the canyons are up to 300 km wide and 10 km deep. Often compared to Earth's Grand Canyon, the Valles Marineris has a very different origin than its tinier, so-called counterpart on Earth. The Grand Canyon is largely a product of water erosion.

  6. Extraterrestrial real estate - Wikipedia

    en.wikipedia.org/wiki/Extraterrestrial_real_estate

    The Moon as seen by an observer from Earth. It is claimed as private property by several individuals. [1] [2]Extraterrestrial real estate refers to claims of land ownership on other planets, natural satellites, or parts of space by certain organizations or individuals.

  7. Composition of Mars - Wikipedia

    en.wikipedia.org/wiki/Composition_of_Mars

    Like Earth, Mars appears to have a molten iron core, or at least a molten outer core. [5] However, there does not appear to be convection in the mantle. Presently Mars shows little geological activity. The elemental composition of Mars is different from Earth's in several significant ways.

  8. Geological history of Mars - Wikipedia

    en.wikipedia.org/wiki/Geological_history_of_Mars

    Generally, this is only known for rocks on Earth. Absolute ages are also known for selected rock units of the Moon based on samples returned to Earth. There is also a proposal to introduce a moment of instability of liquid water. [3] Assigning absolute ages to rock units on Mars is much more problematic.

  9. Orbit of Mars - Wikipedia

    en.wikipedia.org/wiki/Orbit_of_Mars

    Mars comes closer to Earth more than any other planet save Venus at its nearest—56 million km is the closest distance between Mars and Earth, whereas the closest Venus comes to Earth is 40 million km. Mars comes closest to Earth every other year, around the time of its opposition, when Earth is sweeping between the Sun and Mars. Extra-close ...