RR Lupi
Mira variable star in the constellation Lupus
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RR Lupi
Summary
RR Lupi is a Mira variable[1].
Key Facts
- RR Lupi's instance of is recorded as Mira variable[2].
- RR Lupi's constellation is recorded as Lupus[3].
- RR Lupi's spectral class is recorded as M3[4].
- RR Lupi's catalog code is recorded as ASAS J160506-3423.5[5].
- RR Lupi's catalog code is recorded as TYC 7338-1941-1[6].
- RR Lupi's catalog code is recorded as AN 218.1907[7].
- RR Lupi's catalog code is recorded as CSI-34-16018[8].
- RR Lupi's catalog code is recorded as GCRV 65905[9].
- RR Lupi's catalog code is recorded as IRAS 16018-3415[10].
- RR Lupi's catalog code is recorded as SV* HV 3054[11].
- RR Lupi's catalog code is recorded as 2MASS J16050573-3423301[12].
- RR Lupi's catalog code is recorded as Gaia DR2 6035135250894687616[13].
- RR Lupi's catalog code is recorded as RR Lup[14].
- RR Lupi's catalog code is recorded as TIC 94076916[15].
- RR Lupi's type of variable star is recorded as long-period variable star[16].
- RR Lupi's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.53'}[17].
- RR Lupi's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.06'}[18].
- RR Lupi's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.259'}[19].
- RR Lupi's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.131'}[20].
- RR Lupi's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.490'}[21].
- RR Lupi's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.3976'}[22].
- RR Lupi's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.5619'}[23].
- RR Lupi's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-28.0'}[24].
- RR Lupi's Google Knowledge Graph ID is recorded as /g/11p44q4b_1[25].
- RR Lupi's SIMBAD ID is recorded as V* RR Lup[26].
Body
Designation and Status
RR Lupi's instance of is recorded as Mira variable[2].
History and Context
Catalog codes include ASAS J160506-3423.5[5], TYC 7338-1941-1[6], AN 218.1907[7], CSI-34-16018[8], GCRV 65905[9], and IRAS 16018-3415[10].