About: Scarlatti (crater)     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:VolcanicCrater109472413, within Data Space : dbpedia.demo.openlinksw.com associated with source document(s)
QRcode icon
http://dbpedia.demo.openlinksw.com/describe/?url=http%3A%2F%2Fdbpedia.org%2Fresource%2FScarlatti_%28crater%29&invfp=IFP_OFF&sas=SAME_AS_OFF&graph=http%3A%2F%2Fdbpedia.org&graph=http%3A%2F%2Fdbpedia.org

Scarlatti is a pit-floored crater on Mercury, which was discovered in 1974 by the Mariner 10 spacecraft. It has a prominent peak ring, and it is one of 110 peak ring basins on Mercury. The crater floor is covered by the smooth plains material. The crater displays an arcuate collapse feature (central pit) along the northeastern peak ring. The size of the pit, which was first noticed in MESSENGER images obtained in January 2008, is 38 × 12 km. Such a feature may have resulted from collapse of a magma chamber underlying the central peak ring complex of the crater. The collapse feature is an analog of Earth's volcanic calderas. Scarlatti is thought to have the same age as the Caloris basin.

AttributesValues
rdf:type
rdfs:label
  • Scarlatti (cràter) (ca)
  • Scarlatti (cratère) (fr)
  • Cratere Scarlatti (it)
  • Scarlatti (crater) (en)
rdfs:comment
  • Scarlatti est un cratère d'impact présent sur la surface de Mercure. Le cratère fut ainsi nommé par l'Union astronomique internationale en 1979 en hommage aux compositeurs italiens Alessandro et Domenico Scarlatti. Son diamètre est de 132 km. Il se situe dans le (quadrangle H-3) de Mercure. (fr)
  • Scarlatti is a pit-floored crater on Mercury, which was discovered in 1974 by the Mariner 10 spacecraft. It has a prominent peak ring, and it is one of 110 peak ring basins on Mercury. The crater floor is covered by the smooth plains material. The crater displays an arcuate collapse feature (central pit) along the northeastern peak ring. The size of the pit, which was first noticed in MESSENGER images obtained in January 2008, is 38 × 12 km. Such a feature may have resulted from collapse of a magma chamber underlying the central peak ring complex of the crater. The collapse feature is an analog of Earth's volcanic calderas. Scarlatti is thought to have the same age as the Caloris basin. (en)
  • Scarlatti è un cratere da impatto sulla superficie di Mercurio. Il cratere è dedicato ai compositori italiani Alessandro e Domenico Scarlatti, rispettivamente padre e figlio. (it)
  • Scarlatti és un cràter d'impacte en el planeta Mercuri de 132 km de diàmetre. Porta el nom dels compositors italians Domenico Scarlatti (1685-1757) i Alessandro Scarlatti (1660-1725), i el seu nom va ser aprovat per la Unió Astronòmica Internacional el 1979. Va ser descobert el 1974 per la sonda espacial Mariner 10. Es creu que Scarlatti té la mateixa edat que la . (ca)
geo:lat
geo:long
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/Hollows_in_Scarlatti_EN1051805374M.map.jpg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Mariner_10_image_0000142.png
  • http://commons.wikimedia.org/wiki/Special:FilePath/Scarlatti_crater_MESSENGER_WAC_IGF_to_RGB.jpg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Scarlatti_crater_hollows_EN0244488176M_EN0244488181M.jpg
dcterms:subject
Wikipage page ID
Wikipage revision ID
Link from a Wikipage to another Wikipage
sameAs
dbp:wikiPageUsesTemplate
thumbnail
caption
  • Approximate color image by MESSENGER (en)
image size
title
  • Scarlatti (en)
georss:point
  • 40.7 -101.16
has abstract
  • Scarlatti és un cràter d'impacte en el planeta Mercuri de 132 km de diàmetre. Porta el nom dels compositors italians Domenico Scarlatti (1685-1757) i Alessandro Scarlatti (1660-1725), i el seu nom va ser aprovat per la Unió Astronòmica Internacional el 1979. Va ser descobert el 1974 per la sonda espacial Mariner 10. Té un pic anul·lar prominent i el seu sòl està cobert per material llis suau. El cràter mostra una característica de col·lapse arquejat (forat central) al llarg del pic anul·lar. La grandària del forat, que es va veure per primera vegada a les imatges de la sonda espacial MESSENGER obtingudes el gener de 2008, és de 38 × 12 km. Una característica d'aquest tipus pot ser el resultat del col·lapse d'una cambra magmàtica subjacent al pic anul·lar complex del cràter. La característica de col·lapse és anàloga a les calderes volcàniques de la Terra. Es creu que Scarlatti té la mateixa edat que la . (ca)
  • Scarlatti est un cratère d'impact présent sur la surface de Mercure. Le cratère fut ainsi nommé par l'Union astronomique internationale en 1979 en hommage aux compositeurs italiens Alessandro et Domenico Scarlatti. Son diamètre est de 132 km. Il se situe dans le (quadrangle H-3) de Mercure. (fr)
  • Scarlatti is a pit-floored crater on Mercury, which was discovered in 1974 by the Mariner 10 spacecraft. It has a prominent peak ring, and it is one of 110 peak ring basins on Mercury. The crater floor is covered by the smooth plains material. The crater displays an arcuate collapse feature (central pit) along the northeastern peak ring. The size of the pit, which was first noticed in MESSENGER images obtained in January 2008, is 38 × 12 km. Such a feature may have resulted from collapse of a magma chamber underlying the central peak ring complex of the crater. The collapse feature is an analog of Earth's volcanic calderas. Scarlatti is thought to have the same age as the Caloris basin. (en)
  • Scarlatti è un cratere da impatto sulla superficie di Mercurio. Il cratere è dedicato ai compositori italiani Alessandro e Domenico Scarlatti, rispettivamente padre e figlio. (it)
eponym
  • Domenico Scarlatti and Alessandro Scarlatti (en)
globe
  • Mercury (en)
gold:hypernym
prov:wasDerivedFrom
page length (characters) of wiki page
foaf:isPrimaryTopicOf
geo:geometry
  • POINT(-101.16000366211 40.700000762939)
is Link from a Wikipage to another Wikipage of
is Wikipage disambiguates of
is foaf:primaryTopic of
Faceted Search & Find service v1.17_git139 as of Feb 29 2024


Alternative Linked Data Documents: ODE     Content Formats:   [cxml] [csv]     RDF   [text] [turtle] [ld+json] [rdf+json] [rdf+xml]     ODATA   [atom+xml] [odata+json]     Microdata   [microdata+json] [html]    About   
This material is Open Knowledge   W3C Semantic Web Technology [RDF Data] Valid XHTML + RDFa
OpenLink Virtuoso version 08.03.3330 as of Mar 19 2024, on Linux (x86_64-generic-linux-glibc212), Single-Server Edition (378 GB total memory, 58 GB memory in use)
Data on this page belongs to its respective rights holders.
Virtuoso Faceted Browser Copyright © 2009-2024 OpenLink Software