释义 |
- References
{{Starbox begin | name = Rho Lupi }}{{Starbox observe | epoch = J2000.0 | equinox = J2000.0 (ICRS) | constell = Lupus | ra = {{RA|14|37|53.22583}} | dec = {{DEC|−49|25|32.9798}} | appmag_v = 4.05[3] }}{{Starbox character | class = B3/4 V[4] | b-v = −0.15[3] | u-b = −0.56[3] | r-i = | variable = }}{{Starbox astrometry | radial_v = {{Val|8.00|7.40}}[7] | prop_mo_ra = −28.26 | prop_mo_dec = −28.82 | parallax = 10.32 | p_error = 0.16 | parallax_footnote = | absmag_v = −0.88[11] }}{{Starbox detail | source = | mass = 4.66[12] | radius = 3.4[13] | luminosity = 365[14] | temperature = {{Val|15947|542|fmt=commas}}[12] | gravity = | metal_fe = | rotational_velocity = 166[12] | age_myr = 44[12] }}{{Starbox catalog | names = ρ Lup, CD−48° 9198, FK5 3158, HD 128345, HIP 71536, HR 5453, SAO 225071.[18] }}{{Starbox reference | Simbad = rho+Lup }}{{Starbox end}}Rho Lupi, Latinized from ρ Lupi, is a solitary[19] star in the southern constellation of Lupus. It is visible to the naked eye with an apparent visual magnitude of 4.05.[3] Based upon an annual parallax shift of 10.32 mas as seen from Earth, it is located about 316 light years from the Sun. It is a member of the Upper Centaurus Lupus subgroup of the nearby Scorpius–Centaurus Association.[21]This is a B-type main sequence star with a stellar classification of B3/4 V.[4] It is a microvariable with a period of 10.7 hours and an amplitude of 0.0046 in magnitude.[23] With an age of just 44[12] million years, the star is spinning with a projected rotational velocity of 166 km/s.[12] This is giving the star an oblate shape with an equatorial bulge that is an estimated 6% larger than the polar radius.[26] It has an estimated 4.66[12] times the mass of the Sun and about 3.4[13] times the Sun's radius. It is radiating 365[14] times the solar luminosity from its outer atmosphere at an effective temperature of 15,947 K.[12] References1. ^1 {{citation | title=XHIP: An extended hipparcos compilation | last1=Anderson | first1=E. | last2=Francis | first2=Ch. | journal=Astronomy Letters | volume=38 | issue=5 | pages=331 | year=2012 | bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015 | arxiv=1108.4971 | postscript=. }} 2. ^1 {{citation | last1=Koen | first1=Chris | last2=Eyer | first2=Laurent | title=New periodic variables from the Hipparcos epoch photometry | journal=Monthly Notices of the Royal Astronomical Society | volume=331 | pages=45 | year=2002 | doi=10.1046/j.1365-8711.2002.05150.x | bibcode=2002MNRAS.331...45K | arxiv=astro-ph/0112194 | postscript=. }} 3. ^1 2 {{citation | last1=Pasinetti Fracassini | first1=L. 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L. | last2=Iriarte | first2=B. | last3=Mitchell | first3=R. I. | last4=Wisniewskj | first4=W. Z. | title=UBVRIJKL photometry of the bright stars | journal=Communications of the Lunar and Planetary Laboratory | volume=4 | issue=99 | year=1966 | postscript=. | bibcode=1966CoLPL...4...99J | display-authors=1 }} 12. ^1 {{cite simbad | title=rho Lup | accessdate=2017-03-10 | postscript=. }}
[1][2][3][4][5][6][7][8][9][10][11][12] }}{{Stars of Lupus|state=collapsed}} 8 : B-type main-sequence stars|Slowly pulsating B stars|Lupus (constellation)|Bayer objects|Durchmusterung objects|Hipparcos objects|HR objects|Henry Draper Catalogue objects |