NO Apodis

Star in the constellation Apus From Wikipedia, the free encyclopedia

NO Apodis is a solitary,[15] red hued variable star located in the southern circumpolar constellation Apus. It has an average apparent magnitude of 5.86,[16] allowing it to be faintly seen with the naked eye. The object is relatively far at a distance of 790 light years[1] but is drifting closer with a heliocentric radial velocity −18.3 km/s.[7]

A light curve for NO Apodis, plotted from Hipparcos data. The data has been folded with the 24.9 day period listed in the International Variable Star Index.[2]
Right ascension17h 31m 27.4667s[1]
Declination−80° 51 32.876[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
NO Apodis
location of NO Apodis in red
Observation data
Epoch J2000      Equinox J2000
Constellation Apus
Right ascension 17h 31m 27.4667s[1]
Declination −80° 51 32.876[1]
Apparent magnitude (V) 5.71-5.95[2]
Characteristics
Evolutionary stage AGB[3]
Spectral type M3 III[4]
U−B color index +1.80[5]
B−V color index +1.67[5]
Variable type Semiregular[6]
Astrometry
Radial velocity (Rv)−18.3±0.6[7] km/s
Proper motion (μ) RA: −3.662 mas/yr[1]
Dec.: −43.943 mas/yr[1]
Parallax (π)4.1479±0.0741 mas[1]
Distance790 ± 10 ly
(241 ± 4 pc)
Absolute magnitude (MV)−1.32[8]
Details
Mass1.63[9] M
Radius107[10] R
Luminosity1,408[11] L
Surface gravity (log g)1.7±0.1[12] cgs
Temperature3,521±122[10] K
Other designations
59 G. Apodis[13], NO Aps, NSV 8609, CD−80°638, CPD−80°828, FK5 1455, GC 23550, HD 156513, HIP 85760, HR 6429, SAO 258769[14]
Database references
SIMBADdata
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NO Apodis has a stellar classification of M3 III,[4] indicating that it is a red giant. It is currently on the asymptotic giant branch,[3] fusing hydrogen and helium shells around an inert carbon core. At present it has 1.63 times the mass of the Sun[9] and an enlarged radius of 107 R.[10] It shines with a bolometric luminosity 1,408 times that of the Sun[11] from its photosphere at an effective temperature of 3,521 K.[10]

NO Apodis is classified as a semiregular variable of unknown subtype. Observations from Tabur et. al. (2009) reveal it to have two periods, both lasting 26-7 days.[17] During this timeframe, the star flucates between 5.71 and 5.95 in the visual band.[2]

More information Period, Days ...
Periods of NO Apodis[17]
Period Days Amplitude
1 26.2 0.04
2 26.6 0.092
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References

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