dbo:abstract
|
- WASP-43 est une étoile de haute métallicité et de magnitude 12.4, située à environ ∼284 a.l. (∼87,1 pc) dans la constellation du Sextant. (fr)
- WASP-43 is a K-type star in the Sextans constellation. It is about half the size of the Sun, and has approximately half the mass. WASP-43 has one known planet in orbit, a Hot Jupiter called WASP-43b. At the time of publishing of WASP-43b's discovery on April 15, 2011, the planet was the most closely orbiting Hot Jupiter discovered. The small orbit of WASP-43b is thought to be caused by WASP-43's unusually low mass. WASP-43 was first observed between January and May 2009 by the SuperWASP project, and was found to be cooler and slightly richer in metals than the Sun. WASP-43 has also been found to be an active star that rotates at a high velocity. (en)
- WASP-43 — звезда, которая находится в созвездии Секстант на расстоянии приблизительно 260 световых лет от Солнца. Вокруг звезды обращается, как минимум, одна планета. (ru)
|
dbo:wikiPageID
| |
dbo:wikiPageLength
|
- 7466 (xsd:nonNegativeInteger)
|
dbo:wikiPageRevisionID
| |
dbo:wikiPageWikiLink
| |
dbp:ageGyr
| |
dbp:appmagV
| |
dbp:constell
| |
dbp:eccentricity
| |
dbp:epoch
| |
dbp:exoplanet
| |
dbp:gravity
| |
dbp:inclination
| |
dbp:mass
|
- 0.723000 (xsd:double)
- 2.054000 (xsd:double)
|
dbp:metalFe
| |
dbp:pError
| |
dbp:parallax
| |
dbp:period
| |
dbp:radius
|
- 0.674700 (xsd:double)
- 1.049000 (xsd:double)
|
dbp:rotationalVelocity
| |
dbp:semimajor
| |
dbp:temperature
| |
dbp:wikiPageUsesTemplate
| |
dcterms:subject
| |
gold:hypernym
| |
rdf:type
| |
rdfs:comment
|
- WASP-43 est une étoile de haute métallicité et de magnitude 12.4, située à environ ∼284 a.l. (∼87,1 pc) dans la constellation du Sextant. (fr)
- WASP-43 is a K-type star in the Sextans constellation. It is about half the size of the Sun, and has approximately half the mass. WASP-43 has one known planet in orbit, a Hot Jupiter called WASP-43b. At the time of publishing of WASP-43b's discovery on April 15, 2011, the planet was the most closely orbiting Hot Jupiter discovered. The small orbit of WASP-43b is thought to be caused by WASP-43's unusually low mass. WASP-43 was first observed between January and May 2009 by the SuperWASP project, and was found to be cooler and slightly richer in metals than the Sun. WASP-43 has also been found to be an active star that rotates at a high velocity. (en)
- WASP-43 — звезда, которая находится в созвездии Секстант на расстоянии приблизительно 260 световых лет от Солнца. Вокруг звезды обращается, как минимум, одна планета. (ru)
|
rdfs:label
|
- WASP-43 (fr)
- WASP-43 (ja)
- WASP-43 (en)
- WASP-43 (ru)
|
owl:sameAs
| |
prov:wasDerivedFrom
| |
foaf:isPrimaryTopicOf
| |
foaf:name
| |
is dbo:wikiPageWikiLink
of | |
is dbp:star
of | |
is foaf:primaryTopic
of | |