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2MASS J05325346+8246465 (abbreviated 2MASS J0532+8246) is possibly the first brown dwarf observed in the galactic halo of the Milky Way, and the first known substellar subdwarf star. It was discovered from Two Micron All-Sky Survey data, and verified by observations at Palomar Observatory and W. M. Keck Observatory. It has a low metallicity, which indicates it is an old star.

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  • 2MASS J05325346+8246465 (abbreviated 2MASS J0532+8246) is possibly the first brown dwarf observed in the galactic halo of the Milky Way, and the first known substellar subdwarf star. It was discovered from Two Micron All-Sky Survey data, and verified by observations at Palomar Observatory and W. M. Keck Observatory. It has a low metallicity, which indicates it is an old star. The mass and temperature of 2MASS 0532+8246 makes it a rare object in stellar-substellar gap between conventional stars and brown dwarfs. It produces roughly half of its luminosity from hydrogen fusion. Such "gap" objects, covering a narrow range of masses but a wide range of temperatures, and powered by unsteady hydrogen fusion, are exotic but expected to be more common among low-metallicity objects like 2MASS J05325346+8246465. (en)
  • 2MASS J05325346+8246465, auch abgekürzt als 2MASS 0532+8246 bezeichnet, ist ein möglicher L-Unterzwerg im Sternbild Giraffe. Modellenrechnungen ergeben starke Hinweise, dass es sich um ein substellares Objekt unmittelbar unterhalb der Massengrenze für das Wasserstoffbrennen handelt. (de)
  • 2MASS J05325346+8246465는 최초로 발견된 이자 준왜성이다. 현재 수명은 10-15억 년이다. (ko)
  • 2MASS 0532+8246 – brązowy karzeł leżący w gwiazdozbiorze Żyrafy. Należy do typu widmowego sdL7. Jego masa wynosi mniej niż 0,1 masy Słońca, a metaliczność (zawartość pierwiastków cięższych niż hel) zaledwie 0,1 do 0,01 metaliczności Słońca. (pl)
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  • 1049363609 (xsd:integer)
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  • ~10 (en)
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  • 30 (xsd:integer)
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  • 2019-06-10 (xsd:date)
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  • -1.600000 (xsd:double)
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  • 40.236900 (xsd:double)
dbp:temperature
  • 1600 (xsd:integer)
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rdfs:comment
  • 2MASS J05325346+8246465, auch abgekürzt als 2MASS 0532+8246 bezeichnet, ist ein möglicher L-Unterzwerg im Sternbild Giraffe. Modellenrechnungen ergeben starke Hinweise, dass es sich um ein substellares Objekt unmittelbar unterhalb der Massengrenze für das Wasserstoffbrennen handelt. (de)
  • 2MASS J05325346+8246465는 최초로 발견된 이자 준왜성이다. 현재 수명은 10-15억 년이다. (ko)
  • 2MASS 0532+8246 – brązowy karzeł leżący w gwiazdozbiorze Żyrafy. Należy do typu widmowego sdL7. Jego masa wynosi mniej niż 0,1 masy Słońca, a metaliczność (zawartość pierwiastków cięższych niż hel) zaledwie 0,1 do 0,01 metaliczności Słońca. (pl)
  • 2MASS J05325346+8246465 (abbreviated 2MASS J0532+8246) is possibly the first brown dwarf observed in the galactic halo of the Milky Way, and the first known substellar subdwarf star. It was discovered from Two Micron All-Sky Survey data, and verified by observations at Palomar Observatory and W. M. Keck Observatory. It has a low metallicity, which indicates it is an old star. (en)
rdfs:label
  • 2MASS J05325346+8246465 (de)
  • 2MASS J05325346+8246465 (en)
  • 2MASS J05325346+8246465 (ko)
  • 2MASS 0532+8246 (pl)
  • 2MASS 0532+8246 (sv)
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  • 2MASS J05325346+8246465 (en)
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