About: HD 68402

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HD 68402 is a solitary star located in the circumpolar constellation Volans. With an apparent magnitude of 9.09, it is invisible to the naked eye but can be seen with an amateur telescope. This star is located at a distance of 256 light years based on its parallax shift but is drifting away at a rate of 11.60 km/s.

Attributes	Values
rdf:type	Thing place dbo:Location schema:Place celestial body star
rdfs:label	HD 68402 (en) HD 68402 (sv)
rdfs:comment	HD 68402 är en ensam stjärna i den södra delen av stjärnbilden Flygfisken.Den har en skenbar magnitud av ca 9,09 och kräver ett mindre teleskop för att kunna observeras. Baserat på parallax enligt Gaia Data Release 2 på ca 12,7 mas, beräknas den befinna sig på ett avstånd på ca 256 ljusår (ca 79 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 12 km/s. (sv) HD 68402 is a solitary star located in the circumpolar constellation Volans. With an apparent magnitude of 9.09, it is invisible to the naked eye but can be seen with an amateur telescope. This star is located at a distance of 256 light years based on its parallax shift but is drifting away at a rate of 11.60 km/s. (en)
foaf:name	HD68402 (en)
name	HD 68402 (en)
dcterms:subject	Durchmusterung objects G-type main-sequence stars G-type subgiants Henry Draper Catalogue objects Hipparcos objects Planetary systems with one confirmed planet Volans (constellation)
Wikipage page ID	69670271 (xsd:integer)
Wikipage revision ID	1122843640 (xsd:integer)
Link from a Wikipage to another Wikipage	Volans Doppler spectroscopy Durchmusterung objects G-type main-sequence stars G-type subgiants Henry Draper Catalogue objects Hipparcos objects Planetary systems with one confirmed planet Naked eye Photosphere Effective temperature Apparent magnitude Subgiant Henry Draper Catalogue Parallax International Celestial Reference System and Frame J2000.0 Volans (constellation) Kelvin Billion years Sun Circumpolar constellation HARPS Main-sequence star Light years Projected rotational velocity Luminosity of the Sun CORALIE
sameAs	HD 68402 HD 68402 HD 68402
dbp:wikiPageUsesTemplate	dbt:Orbitbox_planet dbt:Notability dbt:Orbitbox_end dbt:Reflist dbt:Short_description dbt:Starbox_astrometry dbt:Starbox_begin dbt:Starbox_catalog dbt:Starbox_character dbt:Starbox_detail dbt:Starbox_end dbt:Starbox_observe dbt:Starbox_reference dbt:Val dbt:DEC dbt:Odlist dbt:RA dbt:Orbitbox_planet_begin dbt:Volans
absmag v	+4.66 (en)
age gyr	1 (xsd:integer)
appmag v	9.090000 (xsd:double)
b-v	+0.68 (en)
class	G5 IV/V (en)
constell	Volans
eccentricity	0.030000 (xsd:double)
EPE	HD+68402 (en)
epoch	J2000.0
equinox	J2000.0 (en)
exoplanet	b (en)
gravity	4.430000 (xsd:double)
mass	1.120000 (xsd:double) ≥3.07 ± 0.35 (en)
metal fe	+0.29 ± 0.10 (en)
NSTED	HD+68402 (en)
p error	0.015500 (xsd:double)
parallax	12.721400 (xsd:double)
period	1103 (xsd:integer)
prop mo dec	+78.935 (en)
prop mo ra	−78.186 (en)
radial v	11.600000 (xsd:double)
radius	1.020000 (xsd:double)
rotational velocity	2.900000 (xsd:double)
semimajor	2.180000 (xsd:double)
Simbad	HD+68402 (en)
temperature	5907 (xsd:integer)
has abstract	HD 68402 is a solitary star located in the circumpolar constellation Volans. With an apparent magnitude of 9.09, it is invisible to the naked eye but can be seen with an amateur telescope. This star is located at a distance of 256 light years based on its parallax shift but is drifting away at a rate of 11.60 km/s. HD 68402 has a classification of G5 IV/V, which indicates that it is a G5 star with the characteristics of a subgiant and main-sequence star. Contrary to its classification, it is actually a G1 dwarf. At present it is slightly more massive than the Sun and has a similar radius to the latter. It radiates at 1.17 times the luminosity of the Sun from its photosphere at an effective temperature of 5,907 K, which gives it a yellow hue. At an age of 1 billion years HD 68402 has a projected rotational velocity of almost 3 km/s and is metal rich like most planetary hosts (1.94 times to be exact). (en) HD 68402 är en ensam stjärna i den södra delen av stjärnbilden Flygfisken.Den har en skenbar magnitud av ca 9,09 och kräver ett mindre teleskop för att kunna observeras. Baserat på parallax enligt Gaia Data Release 2 på ca 12,7 mas, beräknas den befinna sig på ett avstånd på ca 256 ljusår (ca 79 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 12 km/s. (sv)

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