# Llista d'estrelles de l'Orada

Aquesta és una llista d'estrelles notables de la constel·lació de l'Orada, ordenades per ordre decreixent de brillantor.
| Nom | B | HD | HIP | RA | Dec | mag. ap. | mag. abs. | Dist. (al) | Tipus sp. | Notes |
| α Dor | α | 29305 | 21281 | 04$^h$ 33$^m$ 59.72$^s$ | −55° 02′ 42.0″ | 3.30 | −0.36 | 176 | A0IIIp(Si) | estrella doble; variable α² CVn, V$_{max}$ = +3.26$^m$, V$_{min}$ = +3.30$^m$, P = 2.95 d |
| β Dor | β | 37350 | 26069 | 05$^h$ 33$^m$ 37.52$^s$ | −62° 29′ 23.5″ | 3.76 | −3.76 | 1038 | F4-G4Ia-II | variable cefeida, V$_{max}$ = +3.46$^m$, V$_{min}$ = +4.08$^m$, P = 9.8426 d |
| γ Dor | γ | 27290 | 19893 | 04$^h$ 16$^m$ 01.49$^s$ | −51° 29′ 13.5″ | 4.26 | 2.72 | 66 | F0V-F5V | prototip de la variable γ Dor, V$_{max}$ = +4.23$^m$, V$_{min}$ = +4.27$^m$ |
| δ Dor | δ | 39014 | 27100 | 05$^h$ 44$^m$ 46.42$^s$ | −65° 44′ 07.9″ | 4.34 | 1.10 | 145 | A7V | |
| 36 Dor | | 40409 | 27890 | 05$^h$ 54$^m$ 05.90$^s$ | −63° 05′ 27.7″ | 4.65 | 2.47 | 89 | K1III/IV | |
| ζ Dor | ζ | 33262 | 23693 | 05$^h$ 05$^m$ 30.69$^s$ | −57° 28′ 22.8″ | 4.71 | 4.38 | 38 | F7V | |
| θ Dor | θ | 34649 | 24372 | 05$^h$ 13$^m$ 45.43$^s$ | −67° 11′ 07.3″ | 4.81 | −1.31 | 546 | K2III | |
| η² Dor | η² | 43455 | 29353 | 06$^h$ 11$^m$ 15.02$^s$ | −65° 35′ 22.9″ | 5.01 | −1.56 | 671 | M2.5III | |
| ν Dor | ν | 43107 | 29134 | 06$^h$ 08$^m$ 44.34$^s$ | −68° 50′ 36.4″ | 5.06 | 0.42 | 277 | B8V | |
| ε Dor | ε | 39844 | 27534 | 05$^h$ 49$^m$ 53.55$^s$ | −66° 54′ 04.4″ | 5.10 | −0.88 | 512 | B6V | |
| λ Dor | λ | 36189 | 25429 | 05$^h$ 26$^m$ 19.28$^s$ | −58° 54′ 45.4″ | 5.14 | −0.64 | 467 | G6III | |
| WZ Dor | | 33684 | 23840 | 05$^h$ 07$^m$ 34.01$^s$ | −63° 23′ 58.5″ | 5.19 | −1.23 | 627 | M3III | variable semiregular, ΔV = 0.12$^m$, P = 40 d |
| κ Dor | κ | 30478 | 22040 | 04$^h$ 44$^m$ 21.12$^s$ | −59° 43′ 58.2″ | 5.28 | 1.11 | 222 | A8/A9III/IV | |
| 28 Dor | | 37297 | 26001 | 05$^h$ 32$^m$ 59.52$^s$ | −64° 13′ 39.1″ | 5.34 | 1.08 | 232 | G8/K0III | binària espectroscòpica |
| π² Dor | π² | 46116 | 30565 | 06$^h$ 25$^m$ 28.65$^s$ | −69° 41′ 26.8″ | 5.37 | 0.81 | 266 | G8III | |
| π¹ Dor | π¹ | 45669 | 30321 | 06$^h$ 22$^m$ 38.23$^s$ | −69° 59′ 02.9″ | 5.56 | −0.75 | 595 | K5III | |
| R Dor | | 29712 | 21479 | 04$^h$ 36$^m$ 45.68$^s$ | −62° 04′ 37.1″ | 5.59 | 1.61 | 203 | M8IIIe | variable semiregular, V$_{max}$ = +4.8$^m$, V$_{min}$ = +6.6$^m$, P = 338 d |
| η¹ Dor | η¹ | 42525 | 28909 | 06$^h$ 06$^m$ 09.36$^s$ | −66° 02′ 22.9″ | 5.72 | 0.68 | 332 | A0V | |
| | | 36584 | 25482 | 05$^h$ 26$^m$ 59.82$^s$ | −68° 37′ 21.0″ | 6.02 | 1.62 | 248 | F0IV/V | estrella doble |
| | | 27604 | 20109 | 04$^h$ 18$^m$ 39.98$^s$ | −52° 51′ 37.0″ | 6.08 | 1.73 | 242 | A8V+... | estrella doble |
| | | 31746 | 22844 | 04$^h$ 54$^m$ 52.92$^s$ | −58° 32′ 52.1″ | 6.11 | 3.66 | 101 | F3V | |
| | | 36876 | 25781 | 05$^h$ 30$^m$ 15.87$^s$ | −63° 55′ 40.2″ | 6.19 | 0.75 | 400 | F0IV | estrella doble |
| | | 28255 | 20552 | 04$^h$ 24$^m$ 12.32$^s$ | −57° 04′ 16.2″ | 6.28 | 4.12 | 88 | G4V+... | estrella triple |
| AZ Dor | | 37935 | 26368 | 05$^h$ 36$^m$ 54.99$^s$ | −66° 33′ 37.1″ | 6.28 | −0.82 | 856 | B9.5V | estrella Be; variable, V$_{max}$ = 6.26$^m$, V$_{min}$ = 6.29$^m$ |
| | | 46730 | 30973 | 06$^h$ 30$^m$ 03.01$^s$ | −65° 34′ 06.2″ | 6.28 | 1.34 | 317 | F0III | |
| | | 37501 | 26190 | 05$^h$ 34$^m$ 57.44$^s$ | −61° 10′ 33.5″ | 6.32 | 1.18 | 348 | G5IV | |
| 30 Dor | | 38268 | | 05$^h$ 38$^m$ 42.399$^s$ | −69° 06′ 02.81″ | 9.5 | 9.63 | 65.199723 e3 | WR | cúmul d'estrelles RMC 136 |
| | | 39963 | 27660 | 05$^h$ 51$^m$ 23.10$^s$ | −64° 02′ 01.0″ | 6.35 | −1.32 | 1116 | G8III | |
| | | 31754 | 22737 | 04$^h$ 53$^m$ 30.49$^s$ | −66° 40′ 31.6″ | 6.43 | −1.30 | 1148 | M0/M1III | |
| | | 24863 | 18275 | 03$^h$ 54$^m$ 33.94$^s$ | −52° 41′ 25.2″ | 6.46 | 1.31 | 349 | A4V | |
| | | 30610 | 22081 | 04$^h$ 44$^m$ 57.91$^s$ | −63° 13′ 46.9″ | 6.46 | 0.73 | 456 | K0/K1III | |
| AB Dor | | 36705 | 25647 | 05$^h$ 28$^m$ 44.83$^s$ | −65° 26′ 54.9″ | 6.93 | | 49 | K1IIIp... | sistema triple; variable FK Com, V$_{max}$ = +6.77$^m$, V$_{min}$ = +6.98$^m$; membre del grup en moviment AB Doradus |
| HD 28254 | | 28254 | 20606 | 04$^h$ 24$^m$ 50.71$^s$ | −50° 37′ 19.9″ | 7.71 | 3.96 | 183 | G5V | té en planeta (b) |
| HD 30177 | | 30177 | 21850 | 04$^h$ 41$^m$ 54.37$^s$ | −58° 01′ 14.7″ | 8.41 | | 179 | G8V | té un planeta (b) |
| S Dor | | 35343 | | 05$^h$ 18$^m$ 14.3$^s$ | −69° 14′ 59″ | 9.72 | | | A0-5eq | hipergegant en el GNM; prototip de les variables S Dor, V$_{max}$ = +8.6$^m$, V$_{min}$ = +11.5$^m$ |
| HE 0437-5439 | | | | 04$^h$ 38$^m$ 12.77$^s$ | −54° 33′ 11.9″ | 16.3 | | | BV | estrella hiperràpida en el GNM |
| BB Dor | | | | 05$^h$ 29$^m$ 28.66$^s$ | −58° 54′ 46.5″ | | | | | variable semblant a una nova, V$_{max}$ = +14.3$^m$, V$_{min}$ = < +18$^m$ |
| SN 1987A | | | | 05$^h$ 35$^m$ 28.26$^s$ | −69° 16′ 13.0″ | | | | Sm... | supernova in the LMC, V$_{max}$ = +4.75$^m$ |

## Vegeu també

* Llista d'estrelles per constel·lació

## Referències

* ESA. «The Hipparcos and Tycho Catalogues», 1997. Arxivat de l'original el 2006-12-07. [Consulta: 26 desembre 2006].
* Kostjuk, N. D. «HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index», 2002. Arxivat de l'original el 2006-11-24. [Consulta: 26 desembre 2006].
* Roman, N. G. «Identification of a Constellation from a Position», 1987. Arxivat de l'original el 2006-11-24. [Consulta: 26 desembre 2006].
* «SIMBAD Astronomical Database». Centre de Données astronomiques de Strasbourg. [Consulta: 2 gener 2007].