V705 Cassiopeiae, also known as Nova Cassiopeiae 1993 was a nova which erupted in the constellation Cassiopeia during 1993. The nova was discovered at 11:17 UT on 7 December 1993 by amateur astronomer Kazuyoshi Kanatsu of Matsue, Japan, who photographed it using a 35mm camera with a 55mm f/2.8 lens. Asteroid 6976 Kanatsu was named after him in honor of this discovery. At the time of its discovery the nova had a photographic magnitude of 6.5. Around 18 December 1993 it flared briefly to magnitude 5.3 (making it visible to the naked eye), and then it returned rapidly to magnitude 6.5. It underwent a series of smaller flares until mid February 1993, after which it began a precipitous decline in brightness.
| Attributes | Values |
|---|
| rdf:type
| |
| rdfs:label
| - V705 Cassiopeiae (en)
- V705 Cassiopeiae (sv)
|
| rdfs:comment
| - V705 Cassiopeiae eller Nova Cassiopeiae 1993 var en nova i stjärnbilden Cassiopeja. Novan var av magnitud 6,5 när den upptäcktes av Kazuyoshi Kanatsu den 7 december 1993. Novan nådde sitt maximum, +5,6 den 13 december. Därefter bleknade den gradvis till i mitten av februari 1994, när den tappade snabbt i ljusstyrka på samma sätt som DQ Herculi. 18 februari hade den avklingat till magnitud 11 och den 27 februari till magnitud 14,4. Efter att ha nått magnitud 16,0 ökade den åter i ljusstyrka, till magnitud 12,5 i maj 1994. Vid denna ljusstyrka hade den sedan förblivit. (sv)
- V705 Cassiopeiae, also known as Nova Cassiopeiae 1993 was a nova which erupted in the constellation Cassiopeia during 1993. The nova was discovered at 11:17 UT on 7 December 1993 by amateur astronomer Kazuyoshi Kanatsu of Matsue, Japan, who photographed it using a 35mm camera with a 55mm f/2.8 lens. Asteroid 6976 Kanatsu was named after him in honor of this discovery. At the time of its discovery the nova had a photographic magnitude of 6.5. Around 18 December 1993 it flared briefly to magnitude 5.3 (making it visible to the naked eye), and then it returned rapidly to magnitude 6.5. It underwent a series of smaller flares until mid February 1993, after which it began a precipitous decline in brightness. (en)
|
| foaf:depiction
| |
| dcterms:subject
| |
| Wikipage page ID
| |
| Wikipage revision ID
| |
| Link from a Wikipage to another Wikipage
| |
| sameAs
| |
| dbp:wikiPageUsesTemplate
| |
| thumbnail
| |
| appmag v
| |
| constell
| |
| epoch
| |
| has abstract
| - V705 Cassiopeiae, also known as Nova Cassiopeiae 1993 was a nova which erupted in the constellation Cassiopeia during 1993. The nova was discovered at 11:17 UT on 7 December 1993 by amateur astronomer Kazuyoshi Kanatsu of Matsue, Japan, who photographed it using a 35mm camera with a 55mm f/2.8 lens. Asteroid 6976 Kanatsu was named after him in honor of this discovery. At the time of its discovery the nova had a photographic magnitude of 6.5. Around 18 December 1993 it flared briefly to magnitude 5.3 (making it visible to the naked eye), and then it returned rapidly to magnitude 6.5. It underwent a series of smaller flares until mid February 1993, after which it began a precipitous decline in brightness. The light curve of V705 Cassiopeiae showed a very pronounced "dust dip", and its brightness fell to about 16th magnitude in mid March 1994, before rebounding to about magnitude 12.5 where it stayed for about two years, after which it declined further. This dust dip occurs when dust forms as the material ejected in the nova explosion expands and cools. The nova ultimately faded to a quiescent magnitude of 16.4. All novae are binary stars, with a "donor" star orbiting a white dwarf. The two stars are so close to each other that material is passed from the donor star to the white dwarf. The orbital period for the binary that forms V705 Cassiopeiae is 5.472 hours. The white dwarf is estimated to have a mass of 1.05 M☉ and to be receiving 2×10−9 M☉ per year of material from the donor star. (en)
- V705 Cassiopeiae eller Nova Cassiopeiae 1993 var en nova i stjärnbilden Cassiopeja. Novan var av magnitud 6,5 när den upptäcktes av Kazuyoshi Kanatsu den 7 december 1993. Novan nådde sitt maximum, +5,6 den 13 december. Därefter bleknade den gradvis till i mitten av februari 1994, när den tappade snabbt i ljusstyrka på samma sätt som DQ Herculi. 18 februari hade den avklingat till magnitud 11 och den 27 februari till magnitud 14,4. Efter att ha nått magnitud 16,0 ökade den åter i ljusstyrka, till magnitud 12,5 i maj 1994. Vid denna ljusstyrka hade den sedan förblivit. (sv)
|
| prov:wasDerivedFrom
| |
| page length (characters) of wiki page
| |
| foaf:isPrimaryTopicOf
| |
| is Link from a Wikipage to another Wikipage
of | |
| is foaf:primaryTopic
of | |
![[RDF Data]](/fct/images/sw-rdf-blue.png)
![[cxml]](/fct/images/cxml_doc.png)
![[csv]](/fct/images/csv_doc.png)
![[text]](/fct/images/ntriples_doc.png)
![[turtle]](/fct/images/n3turtle_doc.png)
![[ld+json]](/fct/images/jsonld_doc.png)
![[rdf+json]](/fct/images/json_doc.png)
![[rdf+xml]](/fct/images/xml_doc.png)
![[atom+xml]](/fct/images/atom_doc.png)
![[html]](/fct/images/html_doc.png)
