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17 Leporis
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Star in the constellation Lepus
280px
A light curve for SS Leporis, plotted from Hipparcos data
J2000.0
J2000.0 (ICRS)
Lepus
06 04 59.12945
−16 29 03.9692
4.82 to 5.06
A1V + M6III
+0.12 (combined)
+0.24 (combined)
+0.52 (combined)
Z And
+18.74 0.10(center of mass)
−5.955
−3.680
3.5742
0.0992
260.34 1.80 days
4.492 0.014 mas
0.005 0.003
143.7 0.5
162.2 0.7
2448528.78 0.37 HJD commas
203.7 0.4
6.1 1.0
21.32 0.21
A-type star
2.71 0.27
18
9,000
1,900
2.0
M giant
1.30 0.33
66.7 3.3
3,250
1,200
1.0
17 Lep SS Lep −16°1349 41511 28816 2148 151093
17+Lep
17 Leporis is a binary star system in the southern constellation of Lepus. It has an overall apparent visual magnitude which varies between 4.82 and 5.06, making it luminous enough to be visible to the naked eye as a faint star. The variable star designation for this system is SS Leporis, while 17 Leporis is the Flamsteed designation. Parallax measurements yield a distance estimate of around 910 light years from the Sun. The system is moving further away from the Earth with a heliocentric radial velocity of +18.7 km/s.
This is a double-lined spectroscopic binary system with an orbital period of 260 days and an eccentricity of 0.005. The spectrum reveals the pair to consist of an A-type main-sequence star with a stellar classification of A1 V, and a red giant with a class of M6III. The close pair form a symbiotic binary with ongoing mass transfer from the giant to the hotter component. The giant does not appear to be filling its Roche lobe, so the mass transfer is coming from stellar wind off the giant. The pair are surrounded by a shell and a dusty circumbinary disk, with the former obliterating the lines from the A-type star.
Gallery
nolines center File:Zooming in on the unusual double star SS Leporis.ogv This zoom sequence starts with a broad view of the spectacular Milky Way. It then closes in on the small constellation of Lepus (The Hare) and finally focuses on 17 Lep. File:Wide field SS Leporis.jpg Wide field around SS Leporis. The field of view is approximately 2.7 degrees.
References
2991407583086382592
17 Lep 2019-05-31
https://cdsarc.cds.unistra.fr/viz-bin/ftp-index?/ftp/cats/more/HIP/cdroms/cats
Centre de Données astronomiques de Strasbourg /ftp/cats/more/HIP/cdroms/cats
Strasbourg astronomical Data Center 15 October 2022
SS Lep, database entry
http://www.sai.msu.su/groups/cluster/gcvs/gcvs/iii/iii.dat
The combined table of GCVS Vols I-III and NL 67-78 with improved coordinates, General Catalogue of Variable Stars
Sternberg Astronomical Institute
Moscow, Russia
September 9, 2009
June 20, 2017
https://web.archive.org/web/20170620004609/http://www.sai.msu.su/groups/cluster/gcvs/gcvs/iii/iii.dat
dead
§3.1, Direct diameter measurement of a star filling its Roche lobe. The semi-detached binary SS Leporis spatially resolved with VINCI/VLTI
T. Verhoelst E. van Aarle B. Acke
Astronomy and Astrophysics
470 3 August 2007 L21–L24
10.1051/0004-6361:20077840 2007A&A...470L..21V 0705.4410 14471349
http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=V/50/catalog&recno=2148
HR 2148 database entry, The Bright Star Catalogue
5th Revised (Preliminary Version)
D. Hoffleit W. H. Warren, Jr.
CDS
September 9, 2009
Alan D. Welty Richard A. Wade
On the nature of 17 Leporis
The Astronomical Journal
109 1669 January 1995 326–331
10.1086/117276 1995AJ....109..326W free Seet Table 2.
An incisive look at the symbiotic star SS Leporis. Milli-arcsecond imaging with PIONIER/VLTI
1 Blind N.
Boffin H. M. J. Berger J.-P.
Le Bouquin J.-B. Mérand A.
Lazareff B. Zins G.
Astronomy & Astrophysics
536 A55 11 December 2011
10.1051/0004-6361/201118036
2011A&A...536A..55B 1112.1514 118482471
Category:Emission-line stars
Category:Circumstellar disks
Category:Lepus (constellation)
BD-16 1349
Leporis, 17
041511
028816
2148
Leporis, SS
Category:Articles containing video clips
Category:Spectroscopic binaries
Category:A1V stars
Category:M6III stars