U Vulpeculae
{{Short description|Variable star in the constellation Vulpecula}}
{{Starbox begin
| name = U Vulpeculae
}}
{{Starbox image
| image = 250px
| caption = A visual band light curve for U Vulpeculae, adapted from Kiss (1998)
}}
{{Starbox observe
| epoch = J2000.0
| constell = Vulpecula
}}
{{Starbox character
| appmag_1_passband =
| appmag_1 =
| r-i =
| v-r =
| b-v =
| u-b =
| variable = δ Cep
}}
{{Starbox astrometry
| radial_v =
| prop_mo_ra = {{val|0.906|0.050}}
| prop_mo_dec = {{val|−0.960|0.062}}
| parallax = 1.0530
| p_error = 0.0390
}}
{{Starbox orbit
| period_unitless = 2,510 days
| eccentricity = 0.675
| k1 = 3.64
| periastron = 2444800
| periarg = 353
}}
{{Starbox detail
| luminosity =
| rotational_velocity =
}}
{{Starbox catalog
| names = {{odlist | BD=+20° 4200 | HD=185059 | HIP=96458 | HR=7458 | SAO=87447}}
}}
{{Starbox reference
| Simbad = U+Vulpeculae
}}
{{Starbox end}}
U Vulpeculae is a variable and binary star in the constellation Vulpecula. It is not visible to the naked eye, but can be seen with binoculars.
It is a classical Cepheid variable and its apparent magnitude ranges from 6.73 to 7.54 over a precise cycle of 7.99 days. Its variable nature was discovered in 1898 at Potsdam Observatory by Gustav Müller and Paul Kempf.
In 1991 a study of radial velocities showed that it U Vulpeculae is a spectroscopic binary and a full orbit with a period of 2510 days (6.9 years) was first calculated in 1996. The secondary star is invisible and is only known from its effect on the motion of the primary.
References
{{Reflist|refs=
{{cite web | title=U Vulpeculae | url=http://www.aavso.org/vsx/index.php?view=detail.top&oid=38179 | last=Watson | first=Christopher | date=4 January 2010 | work=AAVSO Website | publisher=American Association of Variable Star Observers | access-date=2 August 2015}}
{{cite DR2|1825621002188696448}}
{{cite simbad |title=U Vulpeculae | access-date=2 August 2015}}
}}
{{Stars of Vulpecula}}
{{DEFAULTSORT:U Vulpeculae}}
Category:Classical Cepheid variables