WZ Cephei

{{Short description|Binary star in the constellation Cepheus}}

{{Refimprove|date=February 2018}}

{{Starbox begin

| name = WZ Cephei

}}

{{Starbox image

| image = 250px

| caption = Celestia 1.6.1's impression of WZ Cephei, eclipsing binary of W UMa-type.

}}

{{Starbox observe

| epoch = J2000

| constell = Cepheus

| ra = {{RA|23|22|24.215}}

| dec = {{DEC|+72|54|56.70}}

| appmag_v = +11.22

}}

{{Starbox character

| class = F5V+F5V

| variable=W Ursae Majoris-type

}}

{{Starbox astrometry

| dist_ly = 880.2

| dist_pc = 270{{cite journal | doi=10.1086/498018 | arxiv=astro-ph/0509820| author=Geske | last2=Gettel | first2=S. J. | last3=McKay | first3=T. A.| title=A ROSAT Survey of Contact Binary Stars| journal=The Astronomical Journal| volume=131|issue=1|pages=633–637 |date=2006|bibcode=2006AJ....131..633G| s2cid=7756046}}

}}

{{Starbox detail

| mass = 1.1/0.83

| radius = 1.4/0.82

| luminosity = 3/1

| temperature = 6400

}}

{{Starbox orbit

| period = 0.00114

| axis_unitless = 0.013 AU

| eccentricity = 0.0

| inclination = 86.2{{cite journal| doi=10.1051/aas:1998248| author=Djurasevic| last2=Zakirov| first2=M.| last3=Hojaev| first3=A.| last4=Arzumanyants| first4=G.| title=Analysis of the activity of the eclipsing binary WZ Cephei| journal=Astronomy and Astrophysics Supplement| volume=131| issue=1|pages=17–23 |date=1998|bibcode=1998A&AS..131...17D| doi-access=free}}

}}

{{Starbox catalog

| names = WZ Cep, 2MASS J23222421+7254566, 1RXS J232216.6+725505

}}

{{Starbox reference

| Simbad = WZ+Cep

}}

{{Starbox end}}

WZ Cephei is an eclipsing binary star of W Ursae Majoris-type in the constellation of Cepheus, located 880 light years away from the Sun. The stars orbit around a common orbital barycenter every 0.41744 days (slightly over 10 hours). Timing analyses have revealed the possible presence of a third low-mass stellar companion in a wide orbit.{{cite journal| author=Zhu| author2=Qian| name-list-style=amp| title=WZ Cephei: A Close Binary at the Beginning of Contact Phase| journal=The Astronomical Journal| volume=138|issue=6|pages=2002–2006 |date=2009|bibcode=2009AJ....138.2002Z|doi = 10.1088/0004-6256/138/6/2002 | doi-access=free}}

File:WZCepLightCurve.png for WZ Cephei, plotted from TESS data]]

Heribert Schneller announced the discovery that the star is a variable star, in 1928.

Presence of a third body

According to Zhu & Qian (2009) a third low-mass object of stellar nature could be responsible of orbital period variations observed for WZ Cep with a periodicity of roughly 32 years. Such a companion would yield a minimum mass of 0.17 Solar masses and be located 26.6 Astronomical Units (nearly the same orbital separation of Neptune in Solar System) from the eclipsing binary. The star could likely turn out a Proxima Centauri-analog, with inferred luminosity 3.7 percent that of Sun and 20 percent of its radius, according to mass-radius relationship.

References

{{reflist|refs=

{{cite web |title=MAST: Barbara A. Mikulski Archive for Space Telescopes |url=https://mast.stsci.edu/portal/Mashup/Clients/Mast/Portal.html |publisher=Space Telescope Science Institute |access-date=8 December 2021}}

{{cite journal |last1=Gengler |first1=T. |last2=Blasko |first2=S. |last3=Schneller |first3=H. |title=Mitteilungen uber neue Veranderliche (in German)|journal=Astronomische Nachrichten |date=July 1928 |volume=233 |pages=39-41 |url=https://articles.adsabs.harvard.edu/pdf/1928AN....233...39G |bibcode=1928AN....233...39G |access-date=23 January 2025}}

}}

{{Stars of Cepheus}}

{{DEFAULTSORT:WZ Cephei}}

Category:Cepheus (constellation)

Cephei, WZ

Category:W Ursae Majoris variables

Category:F-type main-sequence stars

{{Var-star-stub}}

{{Multi-star-stub}}