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  1. Mars - Wikipedia

    It is known that in the past, Mars has had a much more circular orbit. At one point, 1.35 million Earth years ago, Mars had an eccentricity of roughly 0.002, much less than that of Earth today. Mars's cycle of eccentricity is 96,000 Earth years compared to Earth's cycle of 100,000 years.

    • 24.007 km/s, (86430 km/h; 53700 mph)
    • 686.971 d, (1.88082 yr; 668.5991 sols)
    • 1.025957 d, 24ʰ 37ᵐ 22.7ˢ
    • 0.636 (0.4–0.87) kPa, 0.00628 atm
  2. Asaph Hall - Wikipedia

    Asaph Hall III (October 15, 1829 – November 22, 1907) was an American astronomer who is most famous for having discovered the two moons of Mars, which are Deimos and Phobos, in 1877. He determined the orbits of satellites of other planets and of double stars, the rotation of Saturn, and the mass of Mars.

  3. 1829 - Wikipedia

    1829 was a common year starting on Thursday of the Gregorian calendar and a common year starting on Tuesday of the Julian calendar, the 1829th year of the Common Era (CE) and Anno Domini (AD) designations, the 829th year of the 2nd millennium, the 29th year of the 19th century, and the 10th and last year of the 1820s decade. As of the start of ...

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  5. Mars cycler - Wikipedia

    EarthMars cyclers with a multiple of 7 synodic periods return to Earth at nearly the same point in its orbit and may encounter Earth and/or Mars multiple times during each cycle. VISIT 1 encounters Earth 3 times and Mars 4 times in 15 years. VISIT 2 encounters Earth 5 times and Mars 2 times in 15 years.

  6. Exploration of Mars - Wikipedia

    Mars 1962A was a Mars flyby mission, launched on October 24, 1962 and Mars 1962B an intended first Mars lander mission, launched in late December of the same year (1962). Both failed from either breaking up as they were going into Earth orbit or having the upper stage explode in orbit during the burn to put the spacecraft into trans-Mars ...

  7. 1899 - Wikipedia

    1899 was a common year starting on Sunday of the Gregorian calendar and a common year starting on Friday of the Julian calendar, the 1899th year of the Common Era (CE) and Anno Domini (AD) designations, the 899th year of the 2nd millennium, the 99th year of the 19th century, and the 10th and last year of the 1890s decade.

  8. Similarities & Differences in Mars & Earth | Sciencing
    • Setting
    • Physical characteristics
    • Climate
    • Geology

    Earth and Mars are planetary neighbors in the solar system, sharing some features, such as a rocky composition, and having differences, such as size and temperature. Although the same materials make up Earth and Mars, they are present in different amounts. The two planets are also thought to have formed at about the same time, although they evolved to become very different. While Earth is home to many forms of life, whether any exists on Mars at all remains a question.

    Both Earth and Mars are believed to have condensed out of a massive cloud of hot gases around the sun about 4.6 billion years ago, according to the European Space Agency. Since that time, both planets slowly cooled and formed into the spherical shapes you see today. Both planets have dense cores and hard exterior crusts. In addition, water had a role in the history of both. Mars is nearly twice as large as the Moon and a little over half the size of Earth, according to the Center for Mars Exploration. The diameter of Mars is about 6,786 kilometers (4,217 miles), compared to that of Earth, which is about 12,756 kilometers (7,926 miles). In addition, Earth has a mass that is 10 times greater. Because of its much smaller size and mass, Mars cooled at a much faster rate than Earth, following its initial formation. Also, its lower gravity resulted in the faster loss of volatile materials, such as water and gases.

    Mars has a very thin atmosphere that consists mostly of carbon dioxide. Average atmospheric pressure is 7 millibars, compared to 1,013 millibars on Earth. Without much atmosphere to protect it from heat loss, temperatures on Mars are much colder. According to NASA Quest, average temperature in the mid-latitudes are minus 50 degrees Celsius (minus 58 degrees Fahrenheit). At night, it can drop to minus 60 degrees Celsius (minus 76 degrees Fahrenheit), while daytime highs may reach 0 degrees Celsius (32 degrees Fahrenheit).

    Although water may once have existed on the surface of Mars, it disappeared long ago for unknown reasons. In comparison, Earth's surface is two-thirds water. The Earth's outer crust is always moving. It is divided into plates that move laterally. In contrast, Mars' is stable, although there still appears to be some magma flow underground. This makes its geologic state very different from Earth's. Greater stability on Mars results in the preservation of much older features, some dating back to about four billion years.

  9. Mars (2016 TV series) - Wikipedia

    Mars is a documentary and hard science fiction television series produced by National Geographic, which premiered on November 14, 2016, on their channel, and FX. Prior to its official air date, it was launched in a streaming format on November 1, 2016.

  10. Mars rover - Wikipedia

    Mars 2, Prop-M rover, 1971, Mars 2 landing failed taking Prop-M with it. The Mars 2 and 3 spacecraft from the Soviet Union had identical 4.5 kg Prop-M rovers. They were to move on skis while connected to the landers with cables. Mars 3, Prop-M rover, 1971, lost when Mars 3 lander stopped communicating about 20 seconds after landing.

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