theta Persei

{{Short description|Star system in the constellation Perseus}}

{{Starbox begin

| name=θ Persei

}}

{{Starbox image

| image=

{{Location mark

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

|label=|position=right

|mark=Red circle.svg|mark_width=10|mark_link=θ Per

|x=730|y=420

}}

|caption=Location of θ Persei (circled)

}}

{{Starbox observe

| epoch=J2000

| constell=Perseus

| ra={{RA|02|44|11.98704}}

| dec={{DEC|+49|13|42.4111}}

| appmag_v=4.11 / 9.987

}}

{{Starbox character

| component1 = θ Per A

| type=Main sequence

| class=F8 V

| b-v=+0.49

| u-b=+0.00

| component2 = θ Per B

| Red dwarf

| class2=M1.5 V

| b-v2=+1.48

| u-b2=

}}

{{Starbox astrometry

| radial_v=+24.32

| prop_mo_ra=+334.66

| prop_mo_dec=-89.99

| parallax=89.87

| p_error=0.22

| parallax_footnote =

| absmag_v=3.88

}}

{{Starbox orbit

| reference =

| period = 2,720

| axis = 22.289

| eccentricity = 0.13

| inclination = 75.44

| node = 128

| periastron = B 1613

| periarg = 100.64

}}

{{Starbox detail

| component1 = θ Per A

| mass = {{val|1.138|0.010}}

| radius = {{val|1.319|0.011}}

| luminosity = {{val|2.235|0.040}}

| temperature = {{val|6,328|86|fmt=commas}}

| metal_fe = {{val|-0.03|0.09}}

| gravity = {{val|4.43|0.17}}

| rotational_velocity =

| age_gyr = {{val|4.0|0.4}}

| component2 = θ Per B

| mass2 = {{val|0.521|0.052}}

| radius2 = {{val|0.498|0.017}}

| temperature2 = {{val|3,685|60|fmt=commas}}

| luminosity2 =

| metal2_fe = {{val|-0.03|0.09}}

| age_gyr2 = 2.4

}}

{{Starbox catalog

| names = θ Per, BD+48°746, GJ 107, CCDM J02441+4913, IDS 02374+4848, WDS J02442+4914

| component1=θ Per A

| names1=13 Persei, HR 799, HD 16895, HIP 12777, FK5 93, GC 3277, PPM 45428, SAO 38288

| component2=θ Per B

| names2=2MASS J02441025+4913540

}}

{{Starbox reference

|Simbad=**+STF+296AB|sn=θ Per

|Simbad2=theta+Per|sn2=θ Per A

|Simbad3=GJ+107+B|sn3=θ Per B

}}

{{Starbox end}}

Theta Persei (Theta Per, θ Persei, θ Per) is a star system 37 light years away from Earth, in the constellation Perseus. It is one of the closest naked-eye stars.

The primary star is a yellowish dwarf (main sequence) star of spectral type F8V, which is somewhat larger and brighter than the Sun, but still within the range considered to have the potential for Earth-like planets. There is also a red dwarf companion of spectral type M1.V, orbiting about 250 AU from the primary. It has a Gaia Data Release 2 parallax of {{val|89.2871|0.1534|ul=mas}}, corresponding to a distance of {{val|11.2|ul=pc}}.

An 11th-magnitude star is listed in double-star catalogues as component C of the multiple system. It was {{val|95|ul="}} away from component A in 2002, although the separation is rapidly increasing as it is a distant background object with a very different proper motion to the other two stars. An unconfirmed companion, possibly a brown dwarf, was reported {{val|6.2|ul="}} from θ Persei B in 2010.

References

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