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15 Aquarii
Star in the constellation Aquarius From Wikipedia, the free encyclopedia
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15 Aquarii, abbreviated 15 Aqr, is a single,[12] blue-white star in the zodiac constellation of Aquarius. 15 Aquarii is the Flamsteed designation. It is a dim star that is just visible to the naked eye under good viewing conditions, having an apparent visual magnitude of 5.83.[2] Based upon an annual parallax shift of 4.6 mas,[1] it is located around 710 light years away. At that distance, the visual magnitude is diminished by an extinction of 0.18 due to interstellar dust.[13] It is moving closer to the Earth with a heliocentric radial velocity of −9 km/s.[5] Relative to its neighbors, 15 Aqr has a peculiar velocity of 28.7+2.9
−3.1 km/s and may (62% chance) be a runaway star.[7]
Hube (1970) found a stellar classification of B7 III[3] for this star, which would suggest it is a B-type giant star. However, the Bright Star Catalogue (1964) listed it as a B-type main-sequence star with a class of B5 V,[4] and multiple sources use this instead.[7][10][8][9] The star is roughly 65[7] million years old with a projected rotational velocity of 20 km/s.[10] It has an estimated 5.7[7] times the mass of the Sun and about 3.4[8] times the Sun's radius. 15 Aquarii is radiating 822[2] times the Sun's luminosity from its photosphere at an effective temperature of 14,318 K.[9]
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