Star in the constellation Apus
NO Apodis
location of NO Apodis in red
Observation dataEpoch J2000 Equinox J2000
Constellation
Apus
Right ascension
17h 31m 27.4667s [ 1]
Declination
−80° 51′ 32.8761″[ 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] Distance 790 ± 10 ly (241 ± 4 pc ) Absolute magnitude (MV )−1.32[ 8]
Details Mass 1.63[ 9] M ☉ Radius 107[ 10] R ☉ Luminosity 1,408[ 11] L ☉ Surface gravity (log g )1.7± 0.1[ 12] cgs Temperature 3,521± 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 SIMBAD data
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]
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]
Periods of NO Apodis[ 17]
Period
Days
Amplitude
1
26.2
0.04
2
26.6
0.092
References
^ a b c d e Brown, A. G. A. ; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties" . Astronomy & Astrophysics . 649 : A1. arXiv :2012.01533 . Bibcode :2021A&A...649A...1G . doi :10.1051/0004-6361/202039657 . S2CID 227254300 . (Erratum: doi :10.1051/0004-6361/202039657e ) . Gaia EDR3 record for this source at VizieR .
^ a b c Watson, Christopher (25 August 2009). "NO Apodis" . The International Variable Star Index . American Association of Variable Star Observers . Retrieved 31 March 2015 .
^ a b Eggen, Olin J. (July 1992). "Asymptotic giant branch stars near the sun". The Astronomical Journal . 104 : 275. Bibcode :1992AJ....104..275E . doi :10.1086/116239 . ISSN 0004-6256 .
^ a b Houk, N.; Cowley, A. P. (1975). University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations −90° to −53° . Bibcode :1975mcts.book.....H .
^ a b Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory . 4 : 99– 110. Bibcode :1966CoLPL...4...99J .
^ Samus’, N. N.; Kazarovets, E. V.; Durlevich, O. V.; Kireeva, N. N.; Pastukhova, E. N. (January 2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports . 61 (1): 80– 88. Bibcode :2017ARep...61...80S . doi :10.1134/S1063772917010085 . ISSN 1063-7729 . S2CID 125853869 .
^ a b Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters . 32 (11): 759– 771. arXiv :1606.08053 . Bibcode :2006AstL...32..759G . doi :10.1134/S1063773706110065 . eISSN 1562-6873 . ISSN 1063-7737 . S2CID 119231169 .
^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters . 38 (5): 331– 346. arXiv :1108.4971 . Bibcode :2012AstL...38..331A . doi :10.1134/S1063773712050015 . eISSN 1562-6873 . ISSN 1063-7737 . S2CID 255204555 .
^ a b Kervella, Pierre; Arenou, Frédéric; Thévenin, Frédéric (2022). "Stellar and substellar companions from Gaia EDR3" . Astronomy & Astrophysics . 657 : A7. arXiv :2109.10912 . Bibcode :2022A&A...657A...7K . doi :10.1051/0004-6361/202142146 . eISSN 1432-0746 . ISSN 0004-6361 .
^ a b c d Stassun, Keivan G.; et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List" . The Astronomical Journal . 158 (4): 138. arXiv :1905.10694 . Bibcode :2019AJ....158..138S . doi :10.3847/1538-3881/ab3467 . ISSN 0004-6256 .
^ a b Brown, A. G. A. ; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties" . Astronomy & Astrophysics . 616 . A1. arXiv :1804.09365 . Bibcode :2018A&A...616A...1G . doi :10.1051/0004-6361/201833051 . Gaia DR2 record for this source at VizieR .
^ Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties" . Astronomy and Astrophysics . 674 : A1. arXiv :2208.00211 . Bibcode :2023A&A...674A...1G . doi :10.1051/0004-6361/202243940 . S2CID 244398875 .
Gaia DR3 record for this source at VizieR .
^ Gould, B. A., Uranometria Argentina , Reprinted and updated by Pilcher, F, archived from the original on 2012-02-27, retrieved 2012-01-06
^ "NO Aps" . SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved July 27, 2022 .
^ Eggleton, P. P.; Tokovinin, A. A. (11 September 2008). "A catalogue of multiplicity among bright stellar systems" . Monthly Notices of the Royal Astronomical Society . 389 (2): 869– 879. arXiv :0806.2878 . Bibcode :2008MNRAS.389..869E . doi :10.1111/j.1365-2966.2008.13596.x . eISSN 1365-2966 . ISSN 0035-8711 .
^ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics . 355 : L27 – L30 . Bibcode :2000A&A...355L..27H . ISSN 0004-6361 .
^ a b Tabur, V.; Bedding, T. R.; Kiss, L. L.; Moon, T. T.; Szeidl, B.; Kjeldsen, H. (21 December 2009). "Long-term photometry and periods for 261 nearby pulsating M giants" . Monthly Notices of the Royal Astronomical Society . 400 (4): 1945– 1961. arXiv :0908.3228 . Bibcode :2009MNRAS.400.1945T . doi :10.1111/j.1365-2966.2009.15588.x . eISSN 1365-2966 . ISSN 0035-8711 .