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
12 - Vallis Rheita
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
Vallis Rheita 42.5°S, 51.5°E
Vallis Rheita is a linear valley, approximately 450 km long (similar to Vallis Snellius). At its widest points it reaches a width of about 30 km. It consists of a string of numerous, partially overlapping craters. It is oriented directly towards the centre of the Nectaris Basin and it is suggested that it may have arisen from secondary events following the Nectaris impact.
The crater chain begins northwest of the crater Rheita, crosses the crater Young (71 km, 41.5°S, 50.9°E), then the crater Mallet (58 km, 45.5°S, 54.2°E) and ends southeast of the crater Reimarus (48 km, 47.7°S, 60.3°E).
Rheita 37.1°S, 47.2°E
Rheita is a prominent crater, 70 km in diameter and with an eccentrically placed central peak, and lies northeast of Metius. Vallis Rheita runs past the crater's southern wall. Slightly farther north lies the crater Rheita E, which, with its measurements of 66 × 30 km, exhibits a very elongated shape. It consists of at least three overlapping individual craters, which probably (like Schiller) gained its current form through a later impact.
If the position of Janssen, Fabricius, Metius, Rheita and Rheita E is examined at a large scale, then it appears that they all lie on a nearly straight line. It is conceivable that their formation, nearly simultaneously, may be traced back to a very large asteroid that broke apart shortly before the impact.
- Type
- Chapter
- Information
- The Cambridge Photographic Moon Atlas , pp. 59 - 60Publisher: Cambridge University PressPrint publication year: 2012