2 Vulpeculae

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

{{Starbox begin

| name = 2 Vulpeculae

}}

{{Starbox image

| image = 250px

| caption = A light curve for ES Vulpeculae, adapted from Lynds (1959)

}}

{{Starbox observe 2s

| epoch = J2000.0

| constell = Vulpecula

| component1 = 2 Vul A

| ra1 = {{RA|19|17|43.6354}}

| dec1 = {{DEC|+23|01|31.9418}}

| appmag_v1 = 5.43

| component2 = 2 Vul B

| ra2 = {{RA|19|17|43.7343}}

| dec2 = {{DEC|+23|01|30.8604}}

| appmag_v2 =

}}

{{Starbox character

| type =

| class = B1 IV

| b-v = {{Val|0.020|0.003}}

| u-b =

| variable = β Cep

}}

{{Starbox astrometry

| component1 = 2 Vul A

| radial_v = {{Val|+1.0|4.2}}

| prop_mo_ra = {{val|+0.956|0.041}}

| prop_mo_dec = {{val|−6.636|0.087}}

| parallax = 1.8212

| p_error = 0.0880

| parallax_footnote =

| absmag_v = −2.35

| component2 = 2 Vul B

| radial_v2 =

| prop_mo_ra2 = {{val|−0.170|0.038}}

| prop_mo_dec2 = {{val|−5.324|0.073}}

| parallax2 = 1.7131

| p_error2 = 0.0757

| parallax_footnote2 =

| absmag_v2 =

}}

{{Starbox detail

| source =

| mass = {{Val|12.5|0.6}}

| radius =

| luminosity_bolometric = 21,922

| temperature = 26,850

| gravity =

| metal_fe = {{Val|−0.06|0.10}}

| rotational_velocity = 270

| age_myr = {{Val|12.6|0.7}}

}}

{{Starbox catalog

| names = {{odlist | V=ES Vul | F=2 Vul | BD=+22°3648 | HD=180968 | HIP=94827 | HR=7318 | SAO=87036 | WDS=19177+2302 }}

}}

{{Starbox reference

| Simbad = 2+Vul

}}

{{Starbox end}}

2 Vulpeculae is a binary star system in the northern constellation of Vulpecula, located around 1,800 light years away from the Sun. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 5.43.

2 Vulpeculae is a double-lined spectroscopic binary; as of 2002, the pair had an angular separation of {{Val|1.72|ul=arcsecond}} along a position angle of 127.2°.

The primary component of the binary is a rapidly rotating Be star with a stellar classification of B1 IV. It is a variable star with an amplitude of 0.06 magnitude and a period of 0.6096 days, tentatively classified as Beta Cephei variable. The variability was discovered in 1959, and it has been assigned the variable star designation ES Vulpeculae.

References

{{Reflist|refs=

{{cite journal

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| date=September 1959 | volume=130 | pages=577–598 | doi=10.1086/146747 | bibcode=1959ApJ...130..577L

| url=https://articles.adsabs.harvard.edu/pdf/1959ApJ...130..577L | access-date=11 September 2024}}

{{cite simbad | title=2 Vul | access-date=2019-03-12 }}

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| bibcode=2017ARep...61...80S | doi=10.1134/S1063772917010085 | s2cid=125853869 }}

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{{Cite Gaia DR3|2022245532721403776}}

{{Cite Gaia DR3|2022245532710961920}}

{{cite journal|bibcode=1959ApJ...130..577L |title=The Light-Variability of Early B Giants |journal=The Astrophysical Journal |volume=130 |page=577 |last1=Lynds |first1=C. R. |year=1959 |doi=10.1086/146747 |doi-access=free }}

}}