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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 ...
The asteroid and comet belts orbit the Sun from the inner rocky planets into outer parts of the Solar System, interstellar space. [16] [17] [18] An astronomical unit, or AU, is the distance from Earth to the Sun, which is approximately 150 billion meters (93 million miles). [19]
Angle distance Planet Elongation to Sun January 17, 2006 02:23:03 Mercury 7°53'south of Venus 6.5° West February 1, 2006 12:13:51 Mercury 1°57' north of Neptune 4.5° East February 14, 2006 15:40:57 Mercury 2' north of Uranus 14.1° East March 26, 2006 21:02:41 Venus 1°52' north of Neptune 46.5° West April 18, 2006 12:27:31 Venus 19' north of
Transits occurring when Mars is at its ascending node take place in May, those at descending node happen in November. This cycle corresponds fairly closely to 151 Mars orbits, 284 Earth orbits, and 133 synodic periods, and is analogous to the cycle of transits of Venus from Earth, which follow a cycle of 243 years (121.5, 8, 105.5, 8). There ...
Volcanism on Venus; Physical characteristics of the Earth Figure of the Earth; Structure of the Earth. Earth's crust; Earth's mantle; Earth's outer core; Earth's inner core; Earth's magnetic field; Atmosphere of Earth; Geology of Earth. Lithosphere of Earth. Plate tectonics; Hydrosphere of Earth Water distribution on Earth; Tides; Physical ...
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Mars Global Surveyor imaged the Earth and Moon on May 8, 2003, 13:00 UTC, very close to maximum angular elongation from the Sun and at a distance of 0.930 AU from Mars. The apparent magnitudes were given as −2.5 and +0.9. [8] At different times the actual magnitudes will vary considerably depending on distance and the phases of the Earth and ...
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