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  2. Crocco's Multiplanetary Trajectory - Wikipedia

    en.wikipedia.org/wiki/Crocco's_Multiplanetary...

    The black Ellipse depicts the trajectory, while the blue, red and green curves represent the Orbits of Earth, Mars and Venus respectively. The positions of the planets are marked on the date of Departure from Earth and at the date the spacecraft passes at the shortest distance to the respective planet.

  3. Geology of solar terrestrial planets - Wikipedia

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

    Earth is the only terrestrial planet known to have an active hydrosphere. 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 ...

  4. Planetary habitability in the Solar System - Wikipedia

    en.wikipedia.org/wiki/Planetary_habitability_in...

    Planetary habitability in the Solar System is the study that searches the possible existence of past or present extraterrestrial life in those celestial bodies. As exoplanets are too far away and can only be studied by indirect means, the celestial bodies in the Solar System allow for a much more detailed study: direct telescope observation, space probes, rovers and even human spaceflight.

  5. Stability of the Solar System - Wikipedia

    en.wikipedia.org/wiki/Stability_of_the_Solar_System

    This could eject it from the Solar System altogether [1] or send it on a collision course with Venus, the Sun, or Earth. [11] Mercury's perihelion-precession rate is dominated by planetplanet interactions, but about 7.5% of Mercury's perihelion precession rate comes from the effects described by general relativity. [12]

  6. Solar System - Wikipedia

    en.wikipedia.org/wiki/Solar_System

    Three of the four inner planets (Venus, Earth, and Mars) have atmospheres substantial enough to generate weather; all have impact craters and tectonic surface features, such as rift valleys and volcanoes. [91] Mercury (0.31–0.59 AU from the Sun) [D 6] is the smallest planet in the Solar System.

  7. How climate change made Venus impossible to inhabit - AOL

    www.aol.com/climate-change-made-venus-impossible...

    Venus currently has a surface temperature of 450℃ (the temperature of an oven’s self-cleaning cycle) and an atmosphere dominated by carbon dioxide (96%) with a density 90 times that of Earth’s.

  8. Terrestrial planet - Wikipedia

    en.wikipedia.org/wiki/Terrestrial_planet

    A terrestrial planet, tellurian 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 .

  9. Perturbation (astronomy) - Wikipedia

    en.wikipedia.org/wiki/Perturbation_(astronomy)

    Gravity Simulator plot of the changing orbital eccentricity of Mercury, Venus, Earth, and Mars over the next 50,000 years. The zero-point on this plot is the year 2007. In the Solar System, many of the disturbances of one planet by another are periodic, consisting of small impulses each time a planet passes another in its orbit.