50 Persei

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

{{Starbox begin}}

{{Starbox image

| image = 250px

| caption = A light curve for V582 Persei, plotted from Hipparcos data

}}

{{Starbox observe

| epoch = J2000.0

| constell = Perseus

| ra = {{RA|04|08|36.61660}}

| dec = {{DEC|+38|02|23.0488}}

| appmag_v = 5.52

}}

{{Starbox character

| class = F7 V

| b-v = +0.54

| u-b = +0.00

| variable = RS CVn and BY Dra

}}

{{Starbox astrometry

| radial_v = +26.2

| prop_mo_ra = +164.10

| prop_mo_dec = −202.60

| parallax = 47.63

| p_error = 0.26

| parallax_footnote =

| absmag_v = 3.87

}}

{{Starbox detail

| mass = 1.16

| radius =

| luminosity =

| gravity = 4.35

| temperature = 6,147

| metal_fe = −0.11

| rotational_velocity = 20.81

| age_gyr = 0.60

}}

{{Starbox catalog

| names = 50 Per, BD+37°882, FK5 2297, GJ 9145, HD 25998, HIP 19335, V582 Persei, HR 1278, SAO 57006.

}}

{{Starbox reference

|Simbad=50+Per

}}

{{Starbox end}}

50 Persei is a star in the constellation Perseus. Its apparent magnitude is 5.52, which is bright enough to be seen with the naked eye. Located around {{convert|21.00|pc|ly}} distant, it is a White main-sequence star of spectral type F7V, a star that is currently fusing its core hydrogen. In 1998 the star was named a candidate Gamma Doradus variable with a period of 3.05 days, which would means it displays variations in luminosity due to non-radial pulsations in the photosphere. Subsequently, it was classified as a RS Canum Venaticorum and BY Draconis variable by an automated program.

This is probably a binary system with an unseen companion. It is physically associated with the likely binary system HIP 19255, with the two pairs orbiting each other over a time scale of around a million years. The components of HIP 19255 have an angular separation of 3.87 and the two components orbit each other every 590 years. 50 Persei may share a gravitational association with Capella, even though the two are separated by nearly 15° − equivalent to a distance of {{Convert|5.9|pc|ly|abbr=on|lk=off|order=flip}}.

50 Persei is emitting an infrared excess at a wavelength of 70 μm, suggesting the presence of a circumstellar debris disk. The disk has a temperature of {{Val|96|5|u=K}}.

References

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{{cite simbad

| title=* 50 Per

| access-date=2016-07-22 }}

}}

{{Stars of Perseus}}

{{DEFAULTSORT:50 Persei}}

Category:Perseus (constellation)

Persei, 50

Category:F-type main-sequence stars

Persei, V582

Category:RS Canum Venaticorum variables

019335

1278

025998

9145

Category:BY Draconis variables

BD+37 0882