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  2. Mare Vaporum - Wikipedia

    en.wikipedia.org/wiki/Mare_Vaporum

    Mare Vaporum / v æ ˈ p ɔːr ə m / (Latin vapōrum, the "sea of vapors") is a lunar mare located between the southwest rim of Mare Serenitatis and the southeast rim of Mare Imbrium. It was named by Giovanni Battista Riccioli in 1651. [2] [3] The mare lies in an old basin or crater that is within the Procellarum basin.

  3. Manilius (crater) - Wikipedia

    en.wikipedia.org/wiki/Manilius_(crater)

    Manilius has a well-defined rim with a sloping inner surface that runs directly down to the ring-shaped mound of scree along the base, and a small outer rampart.The small crater interior has a higher albedo than the surroundings, and it appears bright when the sun is overhead.

  4. List of quadrangles on the Moon - Wikipedia

    en.wikipedia.org/wiki/List_of_quadrangles_on_the...

    The bands are then divided into quadrangles, but unlike the 1:2,500,000 system, the seam is placed at +10° longitude (so 0° longitude is in the middle of a quadrangle), and the numbering within a band starts between −80° and −90°: (±90° to ±80°) 1 quadrangle of 360°, beginning at −80°

  5. Julius Caesar (crater) - Wikipedia

    en.wikipedia.org/wiki/Julius_Caesar_(crater)

    It is located to the west of Mare Tranquillitatis, and directly southeast of the crater Manilius on the Mare Vaporum. To the east is the rounded Sosigenes. The interior floor of Julius Caesar is relatively level, especially in the southwest half. The northern half of the interior has a lower albedo (darker) than the south. Most likely the floor ...

  6. Template:Mars quadrangle layout - Wikipedia

    en.wikipedia.org/wiki/Template:Mars_quadrangle...

    Main page; Contents; Current events; Random article; About Wikipedia; Contact us; Help; Learn to edit; Community portal; Recent changes; Upload file

  7. Lunar mare - Wikipedia

    en.wikipedia.org/wiki/Lunar_mare

    The ages of the mare basalts have been determined both by direct radiometric dating and by the technique of crater counting.The radiometric ages range from about 3.16 to 4.2 billion years old (Ga), [4] whereas the youngest ages determined from crater counting are about 1.2 Ga. [5] Updated measurements of samples collected by the Chang’e-5 mission show that some lunar basalts could be as ...

  8. Module:Celestial object quadrangle - Wikipedia

    en.wikipedia.org/wiki/Module:Celestial_object...

    The following two invocations should produce identical results. (Note that the first has been put through <nowiki> to make the category link visible.) {{#invoke:Celestial object quadrangle|category|globe=mars|lat=80|lon=-10}} → [[Category:Mare Boreum quadrangle]]

  9. Mare Boreum quadrangle - Wikipedia

    en.wikipedia.org/wiki/Mare_Boreum_quadrangle

    Image of the Mare Boreum Quadrangle (MC-1). The region includes the North Polar ice cap, Korolov crater and Chasma Boreale. The Mare Boreum quadrangle is one of a series of 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The Mare Boreum quadrangle is also referred to as MC-1 (Mars ...