e/TVLM513-46546

Information
has gloss	eng: TVLM513-46546 is an ultracool red dwarf in the constellation Boötes, exhibiting a flare star activity and all the same varying semi-regularly due to dissimilarly bright hemispheres and a rotation period of about two days. The star has a mass as low as 90 times the mass of Jupiter (or 9 percent of Sun's mass) and an estimated radius of 11 percent that of Sun (nearly a Jupiter-sized star). The star also shows hints of an unseen companion with undetermined mass. Future monitoring will be able to confirm or rule out low-mass stellar or even planetary mass companions (down to 2-10 Jupiter masses), with orbital periods spanning between 1 and 15 days. . Assuming a stellar luminosity of 0.042 percent that of Sun, the habitable zone where an Earth-like planet may retain liquid water at comfortable temperatures would be located within 0.02 Astronomical Units (roughly 10 times the distance of the Moon from Earth).
lexicalization	eng: TVLM513-46546
instance of	(noun) (astronomy) a celestial body of hot gases that radiates energy derived from thermonuclear reactions in the interior star

Meaning
Castilian
has gloss	spa: \| \|+ TVLM513-46546 \|- \| style="background:#efefef;" align="center" colspan=2\| \|- \|- style="vertical-align: top;" \|Constelación \| Boötes \|- style="vertical-align: top;" \| style="padding-right:1em;" \| Ascensión recta α \| 15h 01min 08.19s \|- style="vertical-align: top;" \|Declinación δ \| +22º 50’ 02.0’’ \|- style="vertical-align: top;" \|Distancia \| 34,6±0,2 años-luz \|- style="vertical-align: top;" \|Magnitud visual \| +11,0 \|- style="vertical-align: top;" \|Magnitud absoluta \| ? \|- style="vertical-align: top;" \|Luminosidad \| 0,0002 soles \|- style="vertical-align: top;" \|Temperatura \| 2200 K \|- style="vertical-align: top;" \|Masa \| 0,09 soles \|- style="vertical-align: top;" \|Tipo espectral \| M8.5 \|} TVLM513-46546 (2MASS J15010818+2250020) es una estrella a 34,6 años luz de distancia de la Tierra en la constelación de Boötes, el pastor. Es una estrella muy tenue de magnitud aparente +11,0, una enana roja de tipo espectral M8.5 en el extremo inferior del límite de masa para las estrellas. Con una temperatura superficial en torno a 2200 K, su masa es de 0,09 masas solares, por lo que efectivamente es una estrella de muy baja masa y no una enana marrón.
lexicalization	spa: TVLM513 46546
lexicalization	spa: TVLM513-46546