Stellae Chamaeleontis
Hic habes indicem stellarum constellationis Chamaeleontis.
Nomen |
B |
F |
HD |
HIP |
Ascensio recta |
Declinatio |
Magn. app. |
Magn. abs. |
Distat (sla) |
Classis spectralis |
Nomina alia; nota |
---|---|---|---|---|---|---|---|---|---|---|---|
α Cha | α | 71243 | 40702 | 08h 18m 31.27s | −76° 55′ 11.9″ | 4.05 | 2.60 | 63 | F5III | ||
γ Cha | γ | 92305 | 51839 | 10h 35m 28.22s | −78° 36′ 28.1″ | 4.11 | −1.40 | 413 | M0III | stella variabilis | |
β Cha | β | 106911 | 60000 | 12h 18m 20.94s | −79° 18′ 44.2″ | 4.24 | −0.36 | 271 | B5Vn | stella variabilis | |
θ Cha | θ | 71701 | 40888 | 08h 20m 38.89s | −77° 29′ 04.5″ | 4.34 | 0.97 | 154 | K0III-IV | stella binaria | |
δ2 Cha | δ2 | 93845 | 52633 | 10h 45m 47.14s | −80° 32′ 24.7″ | 4.45 | −0.79 | 363 | B2.5IV | ||
ε Cha | ε | 104174 | 58484 | 11h 59m 37.69s | −78° 13′ 18.5″ | 4.88 | −0.36 | 364 | B9Vn | stella binaria | |
κ Cha | κ | 104902 | 58905 | 12h 04m 46.66s | −76° 31′ 09.0″ | 5.04 | −0.61 | 441 | K4III | ||
ζ Cha | ζ | 83979 | 46928 | 09h 33m 53.51s | −80° 56′ 28.7″ | 5.07 | −1.02 | 539 | B5V | stella variabilis | |
ι Cha | ι | 82554 | 46107 | 09h 24m 09.73s | −80° 47′ 13.9″ | 5.34 | 1.58 | 184 | F3/F5IV | ||
ν Cha | ν | 85396 | 47956 | 09h 46m 20.42s | −76° 46′ 33.5″ | 5.43 | 1.59 | 191 | G8III | ||
η Cha | η | 75416 | 42637 | 08h 41m 19.60s | −78° 57′ 48.3″ | 5.46 | 0.53 | 316 | B9IV | ||
δ1 Cha | δ1 | 93779 | 52595 | 10h 45m 16.38s | −80° 28′ 10.3″ | 5.46 | 0.28 | 354 | K0III | stella binaria | |
μ Cha | μ | 87971 | 49065 | 10h 00m 43.90s | −82° 12′ 53.1″ | 5.53 | 0.09 | 399 | A0IV | ||
π Cha | π | 101132 | 56675 | 11h 37m 15.94s | −75° 53′ 47.5″ | 5.64 | 2.52 | 137 | F1III | ||
HD 72922 | 72922 | 41191 | 08h 24m 20.38s | −80° 54′ 53.0″ | 5.67 | 1.23 | 252 | G8III | |||
HD 76236 | 76236 | 43012 | 08h 45m 55.23s | −79° 30′ 16.5″ | 5.79 | −0.38 | 559 | K5III | |||
HD 114533 | 114533 | 64587 | 13h 14m 17.36s | −78° 26′ 50.8″ | 5.84 | −2.94 | 1863 | F8Ib | |||
HD 120213 | 120213 | 68009 | 13h 55m 38.99s | −82° 39′ 58.1″ | 5.95 | −1.19 | 872 | K2/K3III:p | |||
DR Cha | 93237 | 52340 | 10h 41m 51.58s | −79° 46′ 59.9″ | 5.97 | −1.46 | 1000 | B5IV | stella variabilis; stella emittens | ||
9 Cha | 9 | 75747 | 42794 | 08h 43m 12.31s | −79° 04′ 12.5″ | 6.05 | 1.10 | 319 | A7V | RS Cha; stella variabilis generis Algol | |
HD 80194 | 80194 | 45166 | 09h 12m 12.27s | −76° 39′ 46.5″ | 6.13 | 0.89 | 364 | K1III | |||
HD 92209 | 92209 | 51835 | 10h 35m 24.80s | −76° 18′ 32.4″ | 6.29 | 0.29 | 517 | K2III | |||
HD 101782 | 101782 | 56996 | 11h 41m 01.60s | −83° 05′ 59.9″ | 6.32 | 1.20 | 344 | K0III | stella binaria | ||
DY Cha | 118285 | 66607 | 13h 39m 12.04s | −75° 41′ 01.6″ | 6.32 | −0.95 | 929 | B8IV | stella variabilis | ||
HD 106248 | 106248 | 59647 | 12h 13m 56.48s | −78° 34′ 26.0″ | 6.34 | 1.17 | 353 | K2/K3IIICN. | |||
HD 115088 | 115088 | 64951 | 13h 18m 48.34s | −79° 58′ 33.5″ | 6.34 | 0.67 | 444 | B9.5/A0V | |||
HD 98617 | 98617 | 55225 | 11h 18m 34.21s | −79° 40′ 07.0″ | 6.35 | 2.30 | 210 | A8IIIm... | |||
HD 94717 | 94717 | 53151 | 10h 52m 28.67s | −79° 33′ 34.0″ | 6.36 | −2.20 | 1680 | K2II/III | |||
HD 101917 | 101917 | 57137 | 11h 42m 54.53s | −79° 18′ 22.9″ | 6.38 | 2.65 | 182 | K0III/IV | |||
HD 99015 | 99015 | 55497 | 11h 21m 57.11s | −77° 36′ 30.1″ | 6.43 | 2.07 | 243 | A5III/IV | |||
HD 113694 | 113694 | 64108 | 13h 08m 20.52s | −78° 26′ 45.5″ | 6.43 | 0.73 | 449 | A0V | stella binaria | ||
HD 86320 | 86320 | 48320 | 09h 51m 00.80s | −80° 03′ 39.9″ | 6.47 | −0.20 | 703 | B8IV | |||
μ2 Cha | μ2 | 88351 | 49326 | 10h 04m 07.37s | −81° 33′ 56.2″ | 6.60 | 0.41 | 564 | G6/G8III | stella variabilis | |
HD 63454 | 63454 | 9.37 | 117 | planetam habet | |||||||
CHXR 73 | 11h 06m 29,3s | -77° 37′ 34″ | 20,2 | 550 | M3 | stella binaria socio singulari |
Nexus externi
recensere- ESA (1997). "The Hipparcos and Tycho Catalogues"
- Kostjuk, N. D. (2002). "HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index"
- Roman, N. G. (1987). "Identification of a Constellation from a Position"
- "SIMBAD Astronomical Database". Centre de Données astronomiques de Strasbourg
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