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16 Camelopardalis
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A-type main sequence star in the constellation Camelopardalis
J2000
05 23 27.84195
+57 32 39.8364
5.28
Camelopardalis
main sequence
A0Vn
−0.03
−0.07
12.0 3.7
+15.396
−54.447
9.3655
0.1506
0.18
2.80 0.04
3.26
96.6 7.2 6.6
9748 92 87 commas
217
400
16 Cam +57°879 2402 34787 25197 1751 25161 J05235+5733A
16+Cam
16 Camelopardalis is a single star in the northern circumpolar constellation Camelopardalis, located 348 light years away from the Sun as determined from parallax measurements. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 5.28. This object is moving further from the Earth with a heliocentric radial velocity of around 12 km/s.
This is an A-type main-sequence star with a stellar classification of A0 Vn, where the 'n' notation indicates "nebulous" lines due to rapid rotation. In the past it was misidentified as a Lambda Boötis star. It is around 400 million years old and is spinning with a projected rotational velocity of 217 km/s. The star has 2.8 times the mass of the Sun and 3.3 times the Sun's radius. It is radiating 97 times the Sun's luminosity from its photosphere at an effective temperature of 9,748 K.
An infrared excess indicates it has a dusty debris disk with a mean temperature of 120 K orbiting at a distance of 52 AU from the star. This disk has a combined mass equal to 2.1% the mass of the Earth.
References
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External links
HR 1751
Image 16 Camelopardalis
CCDM J05234+5732
Category:A-type main-sequence stars
Category:Camelopardalis
Category:Durchmusterung objects
Camelopardalis, 16
034787
025197
1751