page_title: 49 Orionis
hierarchical_section_title: 49 Orionis
caption_attribution_description: Italiano: La stella 49 Orionis e le nebulose IC 429 e IC 430 (talvolta descritte come un unico oggetto). Seppur visivamente adiacenti a 49 Orionis, le nebulose sono associate alla stella variabile V883 Orionis. English: The star 49 Orionis and nebulae IC 429 and IC 430. Both nebulae are not correlated to the star 49 Ori, but to the variable star V883 Orionis.
context_page_description: 49 Orionis is a single star in the equatorial constellation of Orion. It has the Bayer designation d Orionis, while 49 Orionis is the Flamsteed designation. This object is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 4.80. It is located 141 light years away from the Sun based on parallax, but is drifting closer with a radial velocity of −5 km/s.
  In the past 49 Orionis was reported as a spectroscopic binary and an orbit was computed with a period of 445.74 days and an eccentricity of 0.549. But it was later determined to be single.
  This object is an A-type main-sequence star with a stellar classification of A4Vn, where the 'n' suffix indicates broadened "nebulous" lines caused by rapid rotation. It is around 284 million years old with a projected rotational velocity of 186 km/s. This spin is giving the star an oblate shape with an equatorial bulge that is an estimated 8% larger than the polar radius. The star has 1.8 times the mass of the Sun and double the Sun's radius. It is radiating 22 times the Sun's luminosity from its photosphere at an effective temperature of 8,416 K.
context_section_description: 49 Orionis  is a single star in the equatorial constellation of Orion. It has the Bayer designation d Orionis, while 49 Orionis is the Flamsteed designation. This object is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 4.80. It is located 141 light years away from the Sun based on parallax, but is drifting closer with a radial velocity of −5 km/s.
  In the past 49 Orionis was reported as a spectroscopic binary and an orbit was computed with a period of 445.74 days and an eccentricity of 0.549. But it was later determined to be single.
  This object is an A-type main-sequence star with a stellar classification of A4Vn, where the 'n' suffix indicates broadened "nebulous" lines caused by rapid rotation. It is around 284 million years old with a projected rotational velocity of 186 km/s. This spin is giving the star an oblate shape with an equatorial bulge that is an estimated 8% larger than the polar radius. The star has 1.8 times the mass of the Sun and double the Sun's radius. It is radiating 22 times the Sun's luminosity from its photosphere at an effective temperature of 8,416 K.
caption: 49 Orionis (center)
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