Eta Arietis

{{Short description|Star in the constellation Aries}}

{{Starbox begin

| name = η Arietis

}}

{{Starbox image

| image=

{{Location mark

|image=Aries constellation map.svg|alt=|float=center|width=240

|label=|position=right

|mark=Red circle.svg|mark_width=10|mark_link=η Arietis

|x=756|y=424

}}

|caption=Location of η Arietis (circled)

}}

{{Starbox observe

| epoch = J2000

| ra = {{RA|02|12|48.086}}

| dec = {{DEC|+21|12|39.58}}

| appmag_v = 5.227{{±|0.023}}

| constell = Aries

}}

{{Starbox character

| class = F5 V

| b-v = +0.435

| u-b = –0.04{{cn|date=April 2025}}

| variable =

}}

{{Starbox astrometry

| radial_v = +5.38{{±|0.19}}

| prop_mo_ra = +163.917

| prop_mo_dec = +5.000

| pm_footnote =

| parallax = 33.3383

| p_error = 0.1196

| parallax_footnote =

| absmag_v = +2.93

}}

{{Starbox detail

| mass = 1.30{{±|0.19}}

| radius = 1.95{{±|0.08}}

| luminosity = 5.91{{±|0.23}}

| temperature = 6,443{{±|107}}

| gravity = 3.97{{±|0.08}}

| metal_fe = –0.35

| rotational_velocity = 9

| age_gyr = 2.6 Gyr
3.98

}}

{{Starbox catalog

| names = {{odlist | B=η Ari | F=17 Arietis | BD=+20 348 | GJ=1043 | HD=13555 | HIP=10306 | HR=646 | SAO=75204 | GC=2643 | PPM=91445 | TIC=306484795 }}

}}

{{Starbox reference

| Simbad=eta+Ari

}}

{{Starbox end}}

Eta Arietis is a star in the northern constellation of Aries. Its name is a Bayer designation that is Latinized from η Arietis, and abbreviated Eta Ari or η Ari. This star is dimly visible to the naked eye with an apparent visual magnitude of 5.231. Based on an annual parallax shift of {{val|33.34|ul=mas}}, the distance to this star is {{Convert|98|ly|pc|abbr=out|lk=on}}. It is drifting further away from the Sun with a radial velocity of +5 km/s.

This is an ordinary F-type main-sequence star with a stellar classification of F5 V. It is younger than the Sun with an age of about 2.6 billion years, and is spinning with a projected rotational velocity of 9 km/s. This star has 1.3 times the mass of the Sun and double the Sun's radius. It is radiating 5.9 times the luminosity of the Sun from its photosphere at an effective temperature of the outer atmosphere is 6,443 K, giving it the yellow-white-hued glow of an F-type star. The abundance of elements more massive than helium in the stellar atmosphere is lower than in the Sun.

Eta Arietis was examined using the HARPS instrument for radial velocity variations that may be caused by an orbiting companion, but no signal was detected. Nor has an infrared excess been detected using the Spitzer Space Telescope, which might otherwise indicate the presence of circumstellar gas or dust.

References

{{reflist|refs=

{{Cite Gaia DR2|99495498687738624}}

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{{citation | postscript=.

| title=The Revised TESS Input Catalog and Candidate Target List

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| last2=Oelkers | first2=Ryan J. | last3=Paegert | first3=Martin

| last4=Torres | first4=Guillermo | last5=Pepper | first5=Joshua

| last6=Lee | first6=Nathan De | last7=Collins | first7=Kevin

| last8=Latham | first8=David W. | last9=Muirhead | first9=Philip S.

| last10=Chittidi | first10=Jay | last11=Rojas-Ayala | first11=Bárbara

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| journal=The Astronomical Journal | language=en

| volume=158 | issue=4 | pages=138 | date=September 2019

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| arxiv=1905.10694 | bibcode=2019AJ....158..138S

| issn=1538-3881}} [https://vizier.cds.unistra.fr/viz-bin/VizieR-5?-ref=VIZ6818e0e52c4349&-out.add=.&-source=IV/38/tic&-c=033.20035699556%20%2b21.21099376748,eq=J2000,rs=2&-out.orig=o eta Arietis' database entry] at VizieR.

{{cite simbad | title=eta Ari | access-date=2012-08-04}}

}}