Book contents
- Frontmatter
- Preface
- Advice on using this book
- Contents
- The Moon – an introduction
- Atlas of lunar formations
- 1 Mare Smythii
- 2a Mare Crisium
- 2b Mare Crisium
- 3 Cleomedes
- 4 Endymion
- 5 Atlas/Hercules
- 6 Montes Taurus
- 7 Palus Somni
- 8a Mare Fecunditatis
- 8b Mare Fecunditatis
- 9 Langrenus/Petavius
- 10 Mare Australe
- 11 Vlacq
- 12 Vallis Rheita
- 13a Mare Nectaris
- 13b Mare Nectaris
- 14 Rupes Altai
- 15 Abulfeda
- 16 Theophilus
- 17 Sinus Asperitatis
- 18 Statio Tranquillitatis
- 19a Mare Tranquillitatis
- 19b Mare Tranquillitatis
- 20a Mare Serenitatis
- 20b Mare Serenitatis
- 21 Posidonius
- 22 Lacus Mortis
- 23 Aristoteles/Eudoxus
- 24 Montes Caucasus
- 25 Autolycus/Aristillus
- 26 Cassini
- 27 Montes Alpes
- 28 Plato
- 29 Montes Teneriffe
- 30 Archimedes
- 31a Montes Apenninus
- 31b Montes Apenninus
- 32 Mare Vaporum
- 33 Rima Ariadaeus
- 34 Rima Hyginus
- 35 Sinus Medii
- 36 Hipparchus
- 37a Ptolemaeus
- 37b Ptolemaeus
- 38 Rupes Recta
- 39 Regiomontanus
- 40 Maurolycus
- 41 South Pole
- 42 Clavius
- 43 Tycho
- 44 Schiller
- 45 Palus Epidemiarum
- 46 Pitatus
- 47 Mare Nubium
- 48 Fra Mauro
- 49 Mare Cognitum
- 50 Mare Insularum
- 51a Copernicus
- 51b Copernicus
- 52 Eratosthenes
- 53a Mare Imbrium
- 53b Mare Imbrium
- 54 Sinus Iridum
- 55 Gruithuisen
- 56 Mare Frigoris
- 57 North Pole
- 58 Aristarchus
- 59 Kepler
- 60 Seleucus
- 61 Reiner
- 62 Letronne/Hansteen
- 63 Gassendi
- 64 Mare Humorum
- 65 Schickard
- 66 Sirsalis
- 67 Grimaldi
- 68 Mare Orientale
- 69 Lunar Farside
- Glossary
- Index of lunar features
- Image credits
- Further reading and references
7 - Palus Somni
Published online by Cambridge University Press: 05 October 2012
- Frontmatter
- Preface
- Advice on using this book
- Contents
- The Moon – an introduction
- Atlas of lunar formations
- 1 Mare Smythii
- 2a Mare Crisium
- 2b Mare Crisium
- 3 Cleomedes
- 4 Endymion
- 5 Atlas/Hercules
- 6 Montes Taurus
- 7 Palus Somni
- 8a Mare Fecunditatis
- 8b Mare Fecunditatis
- 9 Langrenus/Petavius
- 10 Mare Australe
- 11 Vlacq
- 12 Vallis Rheita
- 13a Mare Nectaris
- 13b Mare Nectaris
- 14 Rupes Altai
- 15 Abulfeda
- 16 Theophilus
- 17 Sinus Asperitatis
- 18 Statio Tranquillitatis
- 19a Mare Tranquillitatis
- 19b Mare Tranquillitatis
- 20a Mare Serenitatis
- 20b Mare Serenitatis
- 21 Posidonius
- 22 Lacus Mortis
- 23 Aristoteles/Eudoxus
- 24 Montes Caucasus
- 25 Autolycus/Aristillus
- 26 Cassini
- 27 Montes Alpes
- 28 Plato
- 29 Montes Teneriffe
- 30 Archimedes
- 31a Montes Apenninus
- 31b Montes Apenninus
- 32 Mare Vaporum
- 33 Rima Ariadaeus
- 34 Rima Hyginus
- 35 Sinus Medii
- 36 Hipparchus
- 37a Ptolemaeus
- 37b Ptolemaeus
- 38 Rupes Recta
- 39 Regiomontanus
- 40 Maurolycus
- 41 South Pole
- 42 Clavius
- 43 Tycho
- 44 Schiller
- 45 Palus Epidemiarum
- 46 Pitatus
- 47 Mare Nubium
- 48 Fra Mauro
- 49 Mare Cognitum
- 50 Mare Insularum
- 51a Copernicus
- 51b Copernicus
- 52 Eratosthenes
- 53a Mare Imbrium
- 53b Mare Imbrium
- 54 Sinus Iridum
- 55 Gruithuisen
- 56 Mare Frigoris
- 57 North Pole
- 58 Aristarchus
- 59 Kepler
- 60 Seleucus
- 61 Reiner
- 62 Letronne/Hansteen
- 63 Gassendi
- 64 Mare Humorum
- 65 Schickard
- 66 Sirsalis
- 67 Grimaldi
- 68 Mare Orientale
- 69 Lunar Farside
- Glossary
- Index of lunar features
- Image credits
- Further reading and references
Summary
Palus Somni 14.1°N, 45.0°E
Palus Somni, ‘Marsh of Dreams’, is a diamond-shaped area, lying immediately west of Proclus. It is completely free from ejecta from the Proclus impact, and the ray system separates Palus Somni from Mare Crisium. Palus Somni extends c. 150 km in an east-west direction and appears to be an intermediate geological stage between a highland and a mare floor. The northern portion is rough and fissured, whereas the southern portion is relatively flat, smooth and level. Palus Somni shows conspicuous nuances of colour, which were formerly the subject of numerous geological studies.
Proclus 16.1°N, 46.8°E
Proclus is a very conspicuous, obviously five-sided crater 28 km in diameter. It lies in the western highlands, adjoining Mare Crisium. The crater walls are sharply defined and seem to be little eroded. The floor of the crater is rough and fissured, and the crater walls reach a height of 2.4 km above the crater floor. Proclus is undoubtedly one of the youngest craters. The asymmetric shape of the impact ejecta is visible when the Moon is 5 to 6 days old, and the illumination around Full Moon causes the ray system to be one of the brightest objects on the lunar surface. The longest ray runs northeast, right across Mare Crisium and is c. 600 km long (that is roughly the distance between Boston and Washington).
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- The Cambridge Photographic Moon Atlas , pp. 47 - 48Publisher: Cambridge University PressPrint publication year: 2012