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Statements

Subject Item
dbr:16_Puppis
rdf:type
yago:WikicatB-typeMain-sequenceStars yago:WikicatB-typeStars dbo:Place dbo:Location yago:Star109444100 yago:NaturalObject100019128 schema:Place yago:CelestialBody109239740 dbo:CelestialBody yago:PhysicalEntity100001930 owl:Thing yago:WikicatFlamsteedObjects dbo:Star yago:Whole100003553 yago:Object100002684
rdfs:label
16 Puppis 16 Puppis 弧矢增十三 16 Puppis
rdfs:comment
船尾座16，又名BD-18 2190，HD 67797、SAO 153890、HR 3192，是船尾座的一颗恒星，视星等为4.4，位于銀經239.04，銀緯7.4，其B1900.0坐标为赤經8h 4m 33.7s，赤緯-18° 7.4′ 8″。 16 Puppis (16 Pup), som är stjärnans Flamsteedbeteckning, är en misstänkt astrometrisk dubbelstjärna belägen i den norra delen av stjärnbilden Akterskeppet. Den har en skenbar magnitud på 4,40 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 7,0 mas, beräknas den befinna sig på ett avstånd på ca 470 ljusår (ca 143 parsek) från solen. 16 Puppis is a suspected astrometric binary star system in the southern constellation of Puppis, and is located in the northernmost part of its constellation, almost due north of the bright star Rho Puppis, and east of Canis Major. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 4.40. The star is located is approximately 465 light years away from the Sun based on parallax. It was the brightest star in Officina Typographica, an obsolete constellation. 16 Puppis è una stella bianco-azzurra nella sequenza principale di magnitudine 4,39 situata nella costellazione della Poppa. Dista 473 anni luce dal sistema solare.
foaf:name
16 Puppis
foaf:depiction
n15:Puppis_constellation_map.svg n15:Red_circle.svg
dcterms:subject
dbc:Hipparcos_objects dbc:Flamsteed_objects dbc:Durchmusterung_objects dbc:Puppis dbc:B-type_main-sequence_stars dbc:B-type_subgiants dbc:Henry_Draper_Catalogue_objects dbc:Bright_Star_Catalogue_objects dbc:Astrometric_binaries
dbo:wikiPageID
38324420
dbo:wikiPageRevisionID
1079515128
dbo:wikiPageWikiLink
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dbpedia-sv:16_Puppis yago-res:16_Puppis dbpedia-it:16_Puppis freebase:m.0q3y5p7 n20:3KF98 dbpedia-zh:弧矢增十三 wikidata:Q3597680
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dbt:Short_description dbt:Odlist dbt:RA dbt:DEC dbt:Reflist dbt:Starbox_begin dbt:Starbox_catalog dbt:Starbox_astrometry dbt:Starbox_reference dbt:Starbox_image dbt:Starbox_observe dbt:Starbox_detail dbt:Starbox_end dbt:Starbox_character dbt:Location_mark dbt:Stars_of_Puppis
dbo:thumbnail
n15:Puppis_constellation_map.svg?width=300
dbp:absmagV
-1.37
dbp:appmagV
4.4
dbp:bV
-0.15
dbp:class
B5 V or B5 IV
dbp:constell
dbr:Puppis_(constellation)
dbp:epoch
J2000
dbp:gravity
3.701
dbp:luminosity
836
dbp:pError
0.22
dbp:parallax
7.01
dbp:propMoDec
−5.55
dbp:propMoRa
−9.87
dbp:radialV
+19.90
dbp:rotationalVelocity
140
dbp:temperature
16680
dbp:uB
-0.6
dbo:abstract
16 Puppis is a suspected astrometric binary star system in the southern constellation of Puppis, and is located in the northernmost part of its constellation, almost due north of the bright star Rho Puppis, and east of Canis Major. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 4.40. The star is located is approximately 465 light years away from the Sun based on parallax. It was the brightest star in Officina Typographica, an obsolete constellation. The visible member is a B-type main-sequence star with a stellar classification of B5 V, according to N. Houk and M. Smith-Moore (1978). Earlier, Hoffleit et al. (1964) had listed a class of B5 IV, suggesting a more evolved subgiant star. It is spinning rapidly, which is creating an equatorial bulge that is 6% larger than the polar radius. The star is radiating 836 times the luminosity of the Sun from its photosphere at an effective temperature of 16,680 K. 16 Puppis è una stella bianco-azzurra nella sequenza principale di magnitudine 4,39 situata nella costellazione della Poppa. Dista 473 anni luce dal sistema solare. 16 Puppis (16 Pup), som är stjärnans Flamsteedbeteckning, är en misstänkt astrometrisk dubbelstjärna belägen i den norra delen av stjärnbilden Akterskeppet. Den har en skenbar magnitud på 4,40 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 7,0 mas, beräknas den befinna sig på ett avstånd på ca 470 ljusår (ca 143 parsek) från solen. 船尾座16，又名BD-18 2190，HD 67797、SAO 153890、HR 3192，是船尾座的一颗恒星，视星等为4.4，位于銀經239.04，銀緯7.4，其B1900.0坐标为赤經8h 4m 33.7s，赤緯-18° 7.4′ 8″。
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dbr:Star
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7214
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