Delta Eridani

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Template:Short description

δ Eridani / Rana
Template:Location mark
Location of δ Eridani (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Eridanus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 3.53[2]
Characteristics
Evolutionary stage Subgiant
Spectral type K0 IV[3]
U−B Template:Engvar +0.69[4]
B−V Template:Engvar +0.92[4]
Variable type none[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[5] km/s
Proper motion (μ) RA: −93.634 mas/yr[1]
Dec.: +744.360 mas/yr[1]
Parallax (π)110.0254±0.1944 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)3.77[6]
Details[7]
MassScript error: No such module "val".[8] Template:Solar mass
RadiusScript error: No such module "val". Template:Solar radius
LuminosityScript error: No such module "val". Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val". cgs
TemperatureScript error: No such module "val". K
Metallicity [Fe/H]Script error: No such module "val". dex
Rotational velocity (v sin i)Script error: No such module "val".[8] km/s
Age6.194[9] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[10]
Database references
SIMBADdata

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Delta Eridani, Latinized from δ Eridani, also named Rana, is the fifth-brightest star in the constellation of Eridanus.

The star is visible to the naked eye with an apparent magnitude of 3.54. It is relatively near to the Sun, with a distance of about 29.6 light-years as determined from parallax.[1] The star is drifting closer with a radial velocity of −6 km/s.[5]

Nomenclature

Delta Eridani is sometimes called Rana;[11] Rana means frog in Latin. This name first appeared as Rana Secunda, the "second frog", in Giuseppe Piazzi's star catalogue; this was likely a misattributed name for Beta Ceti (Diphda), known as the "second frog" in Arabic.[12] The name Rana was approved by the IAU Working Group on Star Names on 4 April 2022.[13]

In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Celestial Meadows, refers to an asterism consisting of δ Eridani, γ Eridani, π Eridani, ε Eridani, ζ Eridani, η Eridani, π Ceti, τ1 Eridani, τ2 Eridani, τ3 Eridani, τ4 Eridani, τ5 Eridani, τ6 Eridani, τ7 Eridani, τ8 Eridani and τ9 Eridani.[14] Consequently, the Chinese name for δ Eridani itself is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx.)[15]

Characteristics

The stellar classification of this star is K0 IV,[3] matching a subgiant star that has exhausted its core hydrogen. This has caused the star to expand and become cooler than a comparable main sequence star. Stellar modelling indicates it is near the end of the subgiant stage and about to transition into a giant. It is an estimated six billion years old[9] with 33% more mass than the Sun.[8] The star has 2.35 times the size of the Sun and is radiating three times the Sun's luminosity from its photosphere at an effective temperature of 5,022 K.[7]

Delta Eridani was catalogued as a suspected RS Canum Venaticorum variable in 1983,[16] varying slightly in brightness between magnitudes 3.51 and 3.56,[17] although subsequent observations did not bear this out[18] and an examination of the star using interferometry did not detect the presence of a companion at the expected distance.[9] Thus, this classification is now considered erroneous.[19] The star has a very low level of chromospheric activity.[19] A low projected rotational velocity of under 1 km/s and the lack of radial velocity variation suggest that this star is being viewed from nearly pole-on.[9]

See also

References

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  14. Template:In lang 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, Template:ISBN.
  15. Template:In lang 香港太空館 - 研究資源 - 亮星中英對照表 Template:Webarchive, Hong Kong Space Museum. Accessed on line November 23, 2010.
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  19. a b Script error: No such module "Citation/CS1".

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External links

Template:Stars of Eridanus