1SWASP J093010.78+533859.5
{{Short description|Quintuple star system in the constellation Ursa Major}}
{{Starbox begin}}
{{Starbox observe 2s
|epoch=J2000
|constell=Ursa Major{{cite constellation|TIC 318210930}}
|component1 = A
|component2 = B
}}
{{Starbox character
|component1 = A
|variable=Algol
|component2 = B
|variable2=W UMa
}}
{{Starbox astrometry
|component1 = A
|parallax=23.5622
|p_error=1.3138
|component2 = B
|parallax2=14.2625
|p_error2=0.0165
}}
{{Starbox orbit
| primary = Aa
| name = Ab
| period_unitless = 31.333 hours
| axis_unitless = {{val|5.762|0.010|ul=solar radius}}
| inclination = {{val|88.2|0.3}}
| eccentricity = 0
}}
{{Starbox orbit
| primary = Ba
| name = Bb
| period_unitless = 5.465 hours
| axis_unitless = {{val|1.665|0.012|ul=solar radius}}
| inclination = {{val|86|4}}
| eccentricity = 0
}}
{{Starbox detail
|component1=J093010Aa
|mass={{val|0.837|0.008}}
|radius={{val|0.832|0.018}}
|temperature={{val|fmt=commas|5185|+25|−20}}
|gravity=4.52
|component2=J093010Ab
|mass2={{val|0.674|0.007}}
|radius2={{val|0.669|0.018}}
|temperature2={{val|fmt=commas|4325|+20|−15}}
|gravity2=4.62
}}
{{Starbox detail|no_heading=y
|component1= J093010Ba
|mass={{val|0.86|0.02}}
|radius={{val|0.79|0.04}}
|temperature={{val|fmt=commas|4700|50}}
|gravity=4.58
|luminosity={{val|6.20|0.05}}
|component2= J093010Bb
|mass2={{val|0.341|0.011}}
|radius2={{val|0.52|0.05}}
|temperature2={{val|fmt=commas|4700|50}}
|gravity2=4.53
|luminosity2={{val|7.12|0.05}}
}}
{{Starbox catalog
|names={{odlist |name=RX J0930.1+5339 |WDS=J09302+5339 }}{{efn|Simbad assigns the 1SWASP J093010.78+533859.5 designation to component B, but various sources make clear it applies to the whole "system" of four or five stars. Similarly, the designation 1SWASP J093012.84+533859.6 is also given to component B, but actually applies to an 18th-magnitude star 18" away.}}
|component2=A
|names2={{odlist |V=V441 UMa |TYC=3807-759-1 }}
|component3=B
|names3={{odlist |V=V442 UMa |TYC=3807-759-2 }}
}}
{{Starbox reference
|Simbad=TIC+318210930
|Simbad2=V441+UMa|sn2=A
|Simbad3=V442+UMa|sn3=B
}}
{{Starbox end}}
1SWASP J093010.78+533859.5 (abbreviated as J093010), also known as V441 Ursae Majoris and V442 Ursae Majoris is a quintuple star system located in the constellation Ursa Major.{{Cite journal|doi= 10.1088/0004-6256/147/5/104|title= 1SWASP J093010.78+533859.5: A Possible Hierarchical Quintuple System|date= 2014|last1= Koo|first1= Jae-Rim|last2= Lee|first2= Jae Woo|last3= Lee|first3= Byeong-Cheol|last4= Kim|first4= Seung-Lee|last5= Lee|first5= Chung-Uk|last6= Hong|first6= Kyeongsoo|last7= Lee|first7= Dong-Joo|last8= Rey|first8= Soo-Chang|journal= The Astronomical Journal|volume= 147|issue= 5|page= 104|arxiv= 1402.4575|bibcode= 2014AJ....147..104K}}{{Cite journal |last1=Lohr |first1=M. E. |last2=Norton |first2=A. J. |last3=Gillen |first3=E. |last4=Busuttil |first4=R. |date=June 12, 2015 |title=The doubly eclipsing quintuple low-mass star system 1SWASP J093010.78+533859.5 |journal=Astronomy & Astrophysics|volume=578 |pages=A103 |doi=10.1051/0004-6361/201525973 |arxiv=1504.07065 |bibcode=2015A&A...578A.103L }} The star system is located approximately 250 light-years from Earth, and was discovered using data from the "Super Wide Angle Search for Planets" (SuperWASP) project in the Canary Islands.
Description
1SWASP J093010.78+533859.5 consists of two pairs of stars, designated J093010A and J093010B respectively, as well as a fifth star. The first pair of stars, J093010A, is a detached eclipsing binary (an Algol variable). The two stars within J093010A orbit with a period of about 1.3 days and are separated by about 5.8 solar radii. The second pair of stars, J093010B is a W Ursae Majoris variable; in this pair the two stars are so close as to be touching each other. The two stars within J093010B take about 5.5 hours (0.2277 days) to orbit each other.{{Cite journal |last=Gazeas |first=K. |date=July 2015 |title=Disentangling the Quadruple System 1SWASP J093010.78+533859.5 |journal=Living Together: Planets|volume=496 |page=112 |bibcode=2015ASPC..496..112G }}
The two pairs J093010A and J093010B are separated by about 1.89 arcseconds, so the separation between the two pairs is likely about 130 astronomical units. The fifth star was detected based on stationary spectral lines coming from the direction of 1SWASP J093010.78+533859.5. The fifth star likely orbits J093010A at a further distance than the eclipsing binary.
Variability
J093010A is a detached (Algol-type) eclipsing binary. Its magnitude drops from a maximum of 9.44 to a primary minimum of 9.75 and a secondary minimum of 9.58 every 1.31 days. It has been given the variable star designation V441 Ursae Majoris.
J093010B is a contact (W UMa-type) eclipsing binary. Its magnitude drops by 0.28 magnitudes at the primary eclipse and 0.25 magnitudes during the secondary eclipse from a maximum magnitude of 10.55. The period is 0.23 days. It has been given the variable star designation V442 Ursae Majoris.
{{Gallery
|title=
|noborder=yes
|align=center
|File:V441UMaLightCurve.png
|A light curve for V441 Ursae Majoris (J093010A), adapted from Lohr et al. (2015). The maximum brightness is the combined light of all 5 stars.
|alt1=
|File:V442UMaLightCurve.png
|A light curve for V442 Ursae Majoris (J093010B), adapted from Lohr et al. (2015). The maximum brightness is the combined light of all 5 stars.
|alt2=
}}
See also
Notes
{{notelist}}
References
{{reflist|refs=
{{cite simbad |title=TIC+318210930 |access-date=2025-07-07 }}
{{cite simbad |title=V441+UMa |access-date=2025-07-07 }}
{{cite simbad |title=V442+UMa |access-date=2025-07-07 }}
{{cite Gaia DR2|1019985085615356672}}
{{cite Gaia DR3|1019985089906439040}}
}}
{{Ursa Major}}
{{2015 in space}}
Category:Wide Angle Search for Planets
Category:K-type main-sequence stars