HD 203949 is a K-type giant star 257 light-years away in the constellation of Microscopium. Its surface temperature is 4618±113 K. It is either on the red giant branch fusing hydrogen in a shell around a helium core, or more likely a red clump star currently fusing helium in its core. HD 203949 is enriched in heavy elements relative to the Sun, with a metallicity ([Fe/H]) of 0.17±0.07 dex. As is common for red giants, HD 203949 has an enhanced concentration of sodium and aluminium compared to iron. Multiplicity surveys did not find any stellar companions around HD 203949 as of 2019.
Attributes | Values |
---|
rdf:type
| |
rdfs:label
| - HD 203949 (en)
- HD 203949 (sv)
- HD 203949 (zh)
|
rdfs:comment
| - HD 203949 is a K-type giant star 257 light-years away in the constellation of Microscopium. Its surface temperature is 4618±113 K. It is either on the red giant branch fusing hydrogen in a shell around a helium core, or more likely a red clump star currently fusing helium in its core. HD 203949 is enriched in heavy elements relative to the Sun, with a metallicity ([Fe/H]) of 0.17±0.07 dex. As is common for red giants, HD 203949 has an enhanced concentration of sodium and aluminium compared to iron. Multiplicity surveys did not find any stellar companions around HD 203949 as of 2019. (en)
- HD 203949 är en ensam stjärna i den mellersta delen av stjärnbilden Mikroskopet. Den har en kombinerad genomsnittlig skenbar magnitud av ca 5,62 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 12,7 mas, beräknas den befinna sig på ett avstånd på ca 257 ljusår (ca 79 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -84 km/s. (sv)
- HD 203949是距離地球257光年,位於顯微鏡座的一顆巨星。它的表面溫度為4618+113− K。它要麼是在紅巨星分支上,在氦核周圍的殼中融合氫氣;要麼更可能是目前在其核心中融合氦的紅群聚恆星。相較於太陽,HD 203949富含重元素,金屬量([Fe/H])為0.17±0.07 。與紅巨星一樣,與鐵相比,HD 203949的鈉和鋁有更高的濃度。 截至2019年,多樣性調查沒有發現HD 203949周圍有任何恆星伴星。 (zh)
|
foaf:name
| |
name
| |
dcterms:subject
| |
Wikipage page ID
| |
Wikipage revision ID
| |
Link from a Wikipage to another Wikipage
| |
sameAs
| |
dbp:wikiPageUsesTemplate
| |
absmag v
| |
age gyr
| |
appmag v
| |
class
| |
constell
| |
eccentricity
| |
epoch
| |
exoplanet
| |
gravity
| |
luminosity bolometric
| |
mass
| |
metal fe
| |
p error
| |
parallax
| |
period
| |
prop mo dec
| |
prop mo ra
| |
radius
| |
semimajor
| |
temperature
| |
type
| |
has abstract
| - HD 203949 is a K-type giant star 257 light-years away in the constellation of Microscopium. Its surface temperature is 4618±113 K. It is either on the red giant branch fusing hydrogen in a shell around a helium core, or more likely a red clump star currently fusing helium in its core. HD 203949 is enriched in heavy elements relative to the Sun, with a metallicity ([Fe/H]) of 0.17±0.07 dex. As is common for red giants, HD 203949 has an enhanced concentration of sodium and aluminium compared to iron. Multiplicity surveys did not find any stellar companions around HD 203949 as of 2019. (en)
- HD 203949 är en ensam stjärna i den mellersta delen av stjärnbilden Mikroskopet. Den har en kombinerad genomsnittlig skenbar magnitud av ca 5,62 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 12,7 mas, beräknas den befinna sig på ett avstånd på ca 257 ljusår (ca 79 parsek) från solen. Den rör sig närmare solen med en heliocentrisk radialhastighet på ca -84 km/s. (sv)
- HD 203949是距離地球257光年,位於顯微鏡座的一顆巨星。它的表面溫度為4618+113− K。它要麼是在紅巨星分支上,在氦核周圍的殼中融合氫氣;要麼更可能是目前在其核心中融合氦的紅群聚恆星。相較於太陽,HD 203949富含重元素,金屬量([Fe/H])為0.17±0.07 。與紅巨星一樣,與鐵相比,HD 203949的鈉和鋁有更高的濃度。 截至2019年,多樣性調查沒有發現HD 203949周圍有任何恆星伴星。 (zh)
|
prov:wasDerivedFrom
| |
page length (characters) of wiki page
| |
foaf:isPrimaryTopicOf
| |
is Link from a Wikipage to another Wikipage
of | |
is Wikipage redirect
of | |
is foaf:primaryTopic
of | |