Geologi Venus

Venus memiliki karakteristik permukaan yang mencolok, yang seindah sewaktu mereka tidak biasa. Mayoritas apa yang kita ketahui hari ini mengenai permukaannya berasal dari pengamatan radar, terutama gambar yang dikirim oleh satelit Magellan dari 16 Agustus 1990, sampai berakhirnya daur orbit ke-6 Magellanm pada September 1994. Sembilan puluh delapan persen permukaan planet ini berhasil dipetakan, 22 persen dari peta itu merupakan gambar stereoskopik tiga dimensi.
Pranala luar
Wikimedia Commons memiliki media mengenai Surface features of Venus.
- Eksplorasi Soviet pada Venus Diarsipkan 2008-08-28 di Wayback Machine.
- Katalog gambar Venus Soviet Diarsipkan 2015-02-24 di Wayback Machine.
- Past missions - Mariner 10 Diarsipkan 2005-09-05 di Wayback Machine.
- The Voyage of Mariner 10 Diarsipkan 2011-01-04 di Wayback Machine.
- Magellan mission to Venus Diarsipkan 2010-12-21 di Wayback Machine.
- Online resources of the Magellan mission to Venus Diarsipkan 2006-05-12 di Wayback Machine.
- Guide for the interpretation of the images taken by Magellan Diarsipkan 2004-02-09 di Wayback Machine.
- Interactive map of Venus Diarsipkan 2006-08-23 di Wayback Machine.
- National Space Science Data Center's Page on Venus (NASA) Diarsipkan 2015-02-10 di Wayback Machine.
- USGS maps of Venus Diarsipkan 2011-06-08 di Wayback Machine.
- NASA/USGS Planetary Geologic Mapping Program Diarsipkan 2010-07-25 di Wayback Machine.
- The Face of Venus: Planetary Geology site Diarsipkan 2010-08-14 di Wayback Machine.
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