Psi3 Aurigae

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

{{DISPLAYTITLE:Psi3 Aurigae}}

{{for|other stars with this Bayer designation|Psi Aurigae{{!}}ψ Aurigae}}

{{Starbox begin

| name = Psi3 Aurigae

}}

{{Starbox image

| image=

{{Location mark

|image=Auriga constellation map.svg|alt=|float=center|width=260

|label=|position=right

|mark=Red circle.svg|mark_width=10|mark_link=ψ3 Aurigae

|x=166|y=420

}}

|caption=Location of ψ3 Aurigae (circled)

}}

{{Starbox observe

| epoch = J2000.0

| equinox = J2000.0 (ICRS)

| constell = Auriga

| ra = {{RA|06|38|49.18001}}

| dec = {{DEC|+39|54|09.2150}}

| appmag_v = +5.20

}}

{{Starbox character

| class = B8 III

| b-v = −0.07

| u-b = −0.38

| r-i =

| variable =

}}

{{Starbox astrometry

| radial_v = {{Val|+9.0|4.2}}

| prop_mo_ra = +27.19

| prop_mo_dec = +16.82

| parallax = 6.34

| p_error = 0.20

| parallax_footnote =

| absmag_v = −2.71

}}

{{Starbox detail

| source =

| mass =

| radius = 4.2

| luminosity = 1,624

| temperature = {{Val|13361|83|fmt=commas}}

| gravity =

| metal_fe =

| rotational_velocity = 118

| age_myr =

}}

{{Starbox catalog

| names = {{odlist | B=ψ3 Aur | F=52 Aur | BD=+40° 1665 | HD=47100 | HIP=31789 | HR=2420 | SAO=59319 }}

}}

{{Starbox reference

| Simbad = psi03+Aur

}}

{{starbox end}}

Psi3 Aurigae, Latinized from ψ3 Aurigae, is a single, blue-white hued star in the northern constellation of Auriga. It is dimly visible to the naked eye with an apparent visual magnitude of +5.20. Based upon an annual parallax shift of {{nowrap|2.38 ± 0.39 mas}} as seen from the Earth, it is approximately {{Convert|1370|ly|pc|abbr=off|lk=on}} distant from the Sun.

This is a B-type giant star with a stellar classification of B8 III. It has about 4.2 and is spinning with a relatively high projected rotational velocity of 118 km/s. The star is radiating 1,624 times the Sun's luminosity from its photosphere at an effective temperature of 13,361 K.

See also

References

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{{citation

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| title=A catalogue of multiplicity among bright stellar systems

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| volume=389 | issue=2 | pages=869–879 | date=September 2008

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{{citation

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{{cite simbad

| title=tet Hyi | access-date=2017-10-13 }}

}}