# Llista d'estrelles del Cranc

La llista d'estrelles del Cranc pretén recollir de forma sintètica i mostrant algunes de les seves principals característiques de les estrelles notables de la Constel·lació del Cranc, ordenades, a priori, per ordre decreixent de brillantor.
| Nom | B | F | Var | HD | HIP | RA | Dec | mag. ap. | mag. abs. | Dist. (al) | Tipus sp. | Notes |
| β Cnc | β | 17 | | 69267 | 40526 | 08$^h$ 16$^m$ 30.95$^s$ | +09° 11′ 08.4″ | 3.53 | −1.22 | 290 | K4III | Al Tarf; estrella variable, ΔV = 0.005$^m$, P = 6.01 d |
| δ Cnc | δ | 47 | | 74442 | 42911 | 08$^h$ 44$^m$ 41.11$^s$ | +18° 09′ 17.5″ | 3.94 | 0.84 | 136 | K0III | Asellus Australis |
| ι Cnc A | ι | 48 | | 74739 | 43103 | 08$^h$ 46$^m$ 41.83$^s$ | +28° 45′ 36.0″ | 4.03 | −0.77 | 298 | G8Iab: | forma part del sistema ι Cnc |
| α Cnc | α | 65 | | 76756 | 44066 | 08$^h$ 58$^m$ 29.20$^s$ | +11° 51′ 28.0″ | 4.26 | 0.63 | 173 | A5m | Acubens, Sertan; probablement variable, V$_{max}$ = 4.20$^m$, V$_{min}$ = 4.27$^m$ |
| γ Cnc | γ | 43 | | 74198 | 42806 | 08$^h$ 43$^m$ 17.21$^s$ | +21° 28′ 06.9″ | 4.66 | 1.23 | 158 | A1IV | Asellus Borealis |
| ζ Cnc | ζ | 16 | | 68255 68256 68257 | 40167 | 08$^h$ 12$^m$ 12.71$^s$ | +17° 38′ 53.3″ | 4.67 | 2.63 | 83 | F7V+F9V +G0V+? | Tegmine, quadruple estrella |
| HD 71115 | | | | 71115 | 41325 | 08$^h$ 25$^m$ 54.79$^s$ | +07° 33′ 52.3″ | 5.13 | −0.08 | 359 | G8II | estrella doble |
| 8 Cnc | | 8 | | 66664 | 39567 | 08$^h$ 05$^m$ 04.51$^s$ | +13° 07′ 06.1″ | 5.14 | 1.09 | 210 | A1V | |
| χ Cnc | χ | 18 | | 69897 | 40843 | 08$^h$ 20$^m$ 03.87$^s$ | +27° 13′ 07.0″ | 5.14 | 3.84 | 59 | F6V | probablement variable |
| ξ Cnc | ξ | 77 | | 78515 | 44946 | 09$^h$ 09$^m$ 21.53$^s$ | +22° 02′ 43.6″ | 5.16 | −0.18 | 380 | K0III | |
| ο¹ Cnc | ο¹ | 62 | | 76543 | 43970 | 08$^h$ 57$^m$ 14.91$^s$ | +15° 19′ 21.8″ | 5.22 | 1.77 | 160 | A5III | variable α² CVn |
| ρ² Cnc | ρ² | 58 | | 76219 | 43834 | 08$^h$ 55$^m$ 39.69$^s$ | +27° 55′ 39.2″ | 5.23 | −1.00 | 574 | G8II-III | |
| σ$^3$ Cnc | σ$^3$ | 64 | | 76813 | 44154 | 08$^h$ 59$^m$ 32.68$^s$ | +32° 25′ 07.1″ | 5.23 | 0.27 | 320 | G9III | probablement variable |
| κ Cnc | κ | 76 | | 78316 | 44798 | 09$^h$ 07$^m$ 44.82$^s$ | +10° 40′ 05.6″ | 5.23 | −0.63 | 484 | B8IIImnp | variable α² CVn, V$_{max}$ = 5.22$^m$, V$_{min}$ = 5.27$^m$, P = 5.0035 d |
| μ² Cnc | μ² | 10 | | 67228 | 39780 | 08$^h$ 07$^m$ 45.84$^s$ | +21° 34′ 55.1″ | 5.30 | 3.46 | 76 | G2IV | |
| θ Cnc | θ | 31 | | 72094 | 41822 | 08$^h$ 31$^m$ 35.77$^s$ | +18° 05′ 40.4″ | 5.33 | −0.57 | 494 | K5III | probablement variable |
| η Cnc | η | 33 | | 72292 | 41909 | 08$^h$ 32$^m$ 42.52$^s$ | +20° 26′ 28.6″ | 5.33 | 0.43 | 312 | K3III | |
| 82 Cnc | π² | 82 | | 79554 | 45410 | 09$^h$ 15$^m$ 13.88$^s$ | +14° 56′ 29.5″ | 5.36 | −1.30 | 701 | K1III | |
| 57 Cnc | | 57 | | 75959 | 43721 | 08$^h$ 54$^m$ 14.70$^s$ | +30° 34′ 45.0″ | 5.40 | 0.15 | 365 | G7III | |
| τ Cnc | τ | 72 | | 78235 | 44818 | 09$^h$ 08$^m$ 00.07$^s$ | +29° 39′ 15.2″ | 5.42 | 0.91 | 260 | G8III | |
| 60 Cnc | | 60 | | 76351 | 43851 | 08$^h$ 55$^m$ 55.56$^s$ | +11° 37′ 33.8″ | 5.44 | −0.82 | 582 | K5III | |
| σ² Cnc | σ² | 59 | | 76398 | 43932 | 08$^h$ 56$^m$ 56.63$^s$ | +32° 54′ 38.1″ | 5.44 | 1.56 | 195 | A7IV | |
| ν Cnc | ν | 69 | | 77350 | 44405 | 09$^h$ 02$^m$ 44.27$^s$ | +24° 27′ 10.6″ | 5.45 | −0.28 | 457 | A0pSi | variable α² CVn, V$_{max}$ = 5.33$^m$, V$_{min}$ = 5.49$^m$, P = 4.20 d |
| 27 Cnc | | 27 | BP | 71250 | 41400 | 08$^h$ 26$^m$ 43.95$^s$ | +12° 39′ 17.5″ | 5.56 | −1.98 | 1052 | M3III | variable semiregular, V$_{max}$ = 5.41$^m$, V$_{min}$ = 5.75$^m$, P = 40 d |
| φ¹ Cnc | φ¹ | 22 | | 71093 | 41377 | 08$^h$ 26$^m$ 27.73$^s$ | +27° 53′ 37.9″ | 5.58 | 0.15 | 398 | K5III | |
| 3 Cnc | | 3 | | 65759 | 39177 | 08$^h$ 00$^m$ 47.31$^s$ | +17° 18′ 31.4″ | 5.60 | −1.12 | 721 | K3III | |
| 15 Cnc | | 15 | BM | 68351 | 40240 | 08$^h$ 13$^m$ 08.87$^s$ | +29° 39′ 23.7″ | 5.62 | −1.52 | 872 | B9p SiCr | variable α² CVn, V$_{max}$ = 5.53$^m$, V$_{min}$ = 5.65$^m$, P = 3.31 d |
| 45 Cnc | A¹ | 45 | | 74228 | 42795 | 08$^h$ 43$^m$ 12.34$^s$ | +12° 40′ 51.1″ | 5.62 | −1.87 | 1028 | A3V+... | probablement variable |
| 49 Cnc | b | 49 | BI | 74521 | 42917 | 08$^h$ 44$^m$ 45.04$^s$ | +10° 04′ 54.2″ | 5.63 | 0.15 | 408 | A1p... | variable α² CVn, V$_{max}$ = 5.58$^m$, V$_{min}$ = 5.71$^m$, P = 6.91 d |
| σ¹ Cnc | σ¹ | 51 | | 75698 | 43584 | 08$^h$ 52$^m$ 34.62$^s$ | +32° 28′ 26.8″ | 5.67 | 1.69 | 204 | A8Vms | probablement variable |
| ο² Cnc | ο² | 63 | | 76582 | 44001 | 08$^h$ 57$^m$ 35.16$^s$ | +15° 34′ 52.4″ | 5.68 | 2.22 | 161 | F0IV | |
| υ¹ Cnc | υ¹ | 30 | | 72041 | 41816 | 08$^h$ 31$^m$ 30.57$^s$ | +24° 04′ 52.4″ | 5.71 | 1.40 | 237 | F0IIIn | probablement variable |
| ψ² Cnc | ψ² | 14 | | 67767 | 40023 | 08$^h$ 10$^m$ 27.23$^s$ | +25° 30′ 29.4″ | 5.73 | 2.61 | 137 | G8IV | probablement variable |
| 1 Cnc | | 1 | | 64960 | 38848 | 07$^h$ 56$^m$ 59.47$^s$ | +15° 47′ 25.4″ | 5.80 | 0.04 | 462 | K3III | |
| HD 69994 | | | | 69994 | 40866 | 08$^h$ 20$^m$ 20.93$^s$ | +20° 44′ 52.2″ | 5.80 | −0.17 | 510 | K1III | |
| HD 77445 | | | | 77445 | 44406 | 09$^h$ 02$^m$ 44.82$^s$ | +07° 17′ 53.7″ | 5.85 | −0.69 | 664 | K3III: | probablement |
| ω¹ Cnc | ω¹ | 2 | | 65714 | 39191 | 08$^h$ 00$^m$ 55.87$^s$ | +25° 23′ 34.2″ | 5.87 | −1.82 | 660 | G8III: | |
| 50 Cnc | A² | 50 | | 74873 | 43121 | 08$^h$ 46$^m$ 56.06$^s$ | +12° 06′ 36.3″ | 5.89 | 1.96 | 199 | A1V | |
| 66 Cnc | | 66 | | 77104 | 44307 | 09$^h$ 01$^m$ 24.13$^s$ | +32° 15′ 08.3″ | 5.89 | −0.08 | 509 | A2V | |
| HD 72945 | | | | 72945 | 42172 | 08$^h$ 35$^m$ 51.05$^s$ | +06° 37′ 13.9″ | 5.91 | 3.79 | 87 | F8V | |
| λ Cnc | λ | 19 | | 70011 | 40881 | 08$^h$ 20$^m$ 32.15$^s$ | +24° 01′ 20.5″ | 5.92 | 0.37 | 419 | B9.5V | |
| 36 Cnc | c | 36 | | 73143 | 42265 | 08$^h$ 37$^m$ 05.79$^s$ | +09° 39′ 20.1″ | 5.92 | 0.17 | 461 | A3V | probablement binària eclipsant |
| 20 Cnc | d¹ | 20 | | 70569 | 41117 | 08$^h$ 23$^m$ 21.87$^s$ | +18° 19′ 56.2″ | 5.94 | 0.52 | 395 | A9V | |
| 29 Cnc | | 29 | | 71555 | 41578 | 08$^h$ 28$^m$ 37.35$^s$ | +14° 12′ 39.1″ | 5.94 | 1.07 | 308 | A5V | |
| 75 Cnc | | 75 | | 78418 | 44892 | 09$^h$ 08$^m$ 47.42$^s$ | +26° 37′ 48.0″ | 5.95 | 3.47 | 102 | G5IV | |
| 1 LMi | | (1) | | 73192 | 42365 | 08$^h$ 38$^m$ 19.00$^s$ | +32° 48′ 07.3″ | 5.96 | 0.70 | 367 | K2III: | |
| 55 Cnc | ρ¹ | 55 | | 75732 | 43587 | 08$^h$ 52$^m$ 36.13$^s$ | +28° 19′ 53.0″ | 5.96 | 5.47 | 41 | G8V | estrella binària; te cinc planetes (b, c, d, e, f) |
| μ¹ Cnc | μ¹ | 9 | BL | 66875 | 39659 | 08$^h$ 06$^m$ 18.40$^s$ | +22° 38′ 07.8″ | 5.97 | −0.45 | 626 | M3III | variable semiregular, V$_{max}$ = 5.97$^m$, V$_{min}$ = 6.04$^m$ |
| 5 Cnc | | 5 | | 65873 | 39236 | 08$^h$ 01$^m$ 30.29$^s$ | +16° 27′ 19.2″ | 5.99 | 0.19 | 472 | B9.5Vn | |
| HD 68461 | | | | 68461 | 40231 | 08$^h$ 12$^m$ 59.74$^s$ | +16° 30′ 51.7″ | 6.03 | −0.02 | 528 | G8III | |
| HD 72617 | | | | 72617 | 42049 | 08$^h$ 34$^m$ 13.35$^s$ | +08° 27′ 08.5″ | 6.04 | 2.22 | 189 | F3IV | |
| 79 Cnc | | 79 | | 78715 | 45033 | 09$^h$ 10$^m$ 20.86$^s$ | +21° 59′ 47.1″ | 6.04 | 0.49 | 420 | G8III | |
| RS Cnc | | | RS | 78712 | 45058 | 09$^h$ 10$^m$ 38.81$^s$ | +30° 57′ 47.6″ | 6.04 | 0.61 | 397 | M6S | estel de tecneci; variable semiregular, V$_{max}$ = 5.33$^m$, V$_{min}$ = 6.94$^m$, P = 242.2 d |
| HD 65257 | | | | 65257 | 38975 | 07$^h$ 58$^m$ 31.48$^s$ | +16° 31′ 07.3″ | 6.05 | −2.11 | 1399 | K0 | probablement variable |
| HD 65522 | | | | 65522 | 39067 | 07$^h$ 59$^m$ 35.07$^s$ | +13° 14′ 31.9″ | 6.05 | 1.22 | 301 | K2 | |
| 28 Cnc | | 28 | CX | 71496 | 41574 | 08$^h$ 28$^m$ 36.80$^s$ | +24° 08′ 42.2″ | 6.05 | 1.45 | 271 | F0Vn | variable δ Sct, ΔV = 0.025$^m$, P = 0.096 d |
| 67 Cnc | | 67 | | 77190 | 44342 | 09$^h$ 01$^m$ 48.88$^s$ | +27° 54′ 10.0″ | 6.07 | 2.23 | 191 | A8Vn | probablement variable |
| HD 68099 | | | | 68099 | 40085 | 08$^h$ 11$^m$ 16.60$^s$ | +09° 49′ 16.6″ | 6.08 | −1.06 | 872 | B6III | |
| 21 Cnc | | 21 | | 70734 | 41163 | 08$^h$ 23$^m$ 55.21$^s$ | +10° 37′ 55.6″ | 6.11 | −1.56 | 1113 | M2III | probablement variable |
| 25 Cnc | d² | 25 | | 71030 | 41319 | 08$^h$ 25$^m$ 49.99$^s$ | +17° 02′ 47.9″ | 6.11 | 2.85 | 147 | F6V | |
| 46 Cnc | | 46 | | 74485 | 42954 | 08$^h$ 45$^m$ 21.42$^s$ | +30° 41′ 51.9″ | 6.12 | 0.30 | 477 | G5III | |
| φ² Cnc A | φ² | 23 | | 71150 | 41404 | 08$^h$ 26$^m$ 47.08$^s$ | +26° 56′ 07.7″ | 6.14 | 1.50 | 276 | A3V | forma part del sistema φ² Cnc; probablement variable |
| HD 80546 | | | | 80546 | 45896 | 09$^h$ 21$^m$ 27.17$^s$ | +32° 54′ 07.9″ | 6.16 | 1.22 | 317 | K3III | |
| HD 76508 | | | | 76508 | 43957 | 08$^h$ 57$^m$ 08.30$^s$ | +17° 08′ 37.8″ | 6.17 | 0.82 | 384 | K1III | |
| φ² Cnc B | φ² | 23 | | 71151 | | 08$^h$ 26$^m$ 47.00$^s$ | +26° 56′ 07.0″ | 6.19 | 1.55 | 276 | A6V | forma part del sistema φ² Cnc |
| HD 76629 | | | | 76629 | 44010 | 08$^h$ 57$^m$ 42.03$^s$ | +09° 23′ 16.0″ | 6.19 | −1.15 | 956 | G8III | |
| HD 66552 | | | | 66552 | 39535 | 08$^h$ 04$^m$ 45.32$^s$ | +18° 50′ 31.4″ | 6.21 | 1.40 | 299 | B9V | |
| HD 66684 | | | | 66684 | 39607 | 08$^h$ 05$^m$ 37.05$^s$ | +27° 31′ 47.1″ | 6.21 | −1.08 | 934 | A0V | probablement variable, V$_{max}$ = 6.16$^m$, V$_{min}$ = 6.21$^m$ |
| 4 LMi | | (4) | | 73596 | 42538 | 08$^h$ 40$^m$ 18.31$^s$ | +31° 56′ 31.1″ | 6.21 | 1.05 | 350 | F5III | probablement variable |
| HD 67959 | | | | 67959 | 40058 | 08$^h$ 10$^m$ 58.90$^s$ | +14° 37′ 46.3″ | 6.22 | −0.04 | 581 | A1V | |
| 12 Cnc | | 12 | | 67483 | 39874 | 08$^h$ 08$^m$ 42.44$^s$ | +13° 38′ 27.4″ | 6.25 | 1.59 | 278 | F3V | |
| 53 Cnc | | 53 | BO | 75716 | 43575 | 08$^h$ 52$^m$ 28.60$^s$ | +28° 15′ 33.0″ | 6.25 | −0.92 | 886 | M3III | variable irregular lenta, V$_{max}$ = 5.9$^m$, V$_{min}$ = 6.37$^m$ |
| 61 Cnc | | 61 | | 76572 | 44031 | 08$^h$ 57$^m$ 58.63$^s$ | +30° 14′ 01.5″ | 6.25 | 2.75 | 164 | F6V | |
| HD 72505 | | | | 72505 | 42010 | 08$^h$ 33$^m$ 45.06$^s$ | +13° 15′ 26.7″ | 6.26 | 1.40 | 306 | K0III | |
| HD 69478 | | | | 69478 | 40617 | 08$^h$ 17$^m$ 31.66$^s$ | +08° 51′ 58.8″ | 6.28 | −1.28 | 1062 | G8III | |
| ε Cnc | ε | 41 | | 73731 | 42556 | 08$^h$ 40$^m$ 27.03$^s$ | +19° 32′ 41.4″ | 6.29 | 0.16 | 548 | Am | pertany al Cúmul del pessebre |
| HD 65735 | | | | 65735 | 39180 | 08$^h$ 00$^m$ 48.10$^s$ | +19° 48′ 58.4″ | 6.30 | 1.18 | 345 | K1III | |
| FZ Cnc | | | FZ | 76830 | 44126 | 08$^h$ 59$^m$ 10.76$^s$ | +18° 08′ 06.1″ | 6.30 | −0.35 | 697 | M4IIIvar | variable semiregular |
| 4 Cnc | ω² | 4 | | 65856 | 39263 | 08$^h$ 01$^m$ 43.77$^s$ | +25° 05′ 22.0″ | 6.32 | 0.00 | 598 | A1V | |
| HD 72943 | | | | 72943 | 42187 | 08$^h$ 36$^m$ 07.71$^s$ | +15° 18′ 49.3″ | 6.33 | 1.77 | 267 | F0IV | |
| HD 65757 | | | | 65757 | 39194 | 08$^h$ 01$^m$ 00.79$^s$ | +23° 34′ 59.4″ | 6.34 | 1.70 | 276 | K1III-IV | |
| υ² Cnc | υ² | 32 | | 72324 | 41940 | 08$^h$ 33$^m$ 00.14$^s$ | +24° 05′ 05.7″ | 6.35 | 0.80 | 421 | G9III | |
| 54 Cnc | | 54 | | 75528 | 43454 | 08$^h$ 51$^m$ 01.53$^s$ | +15° 21′ 01.7″ | 6.36 | 3.35 | 130 | G2IV | |
| HD 68776 | | | | 68776 | 40354 | 08$^h$ 14$^m$ 21.01$^s$ | +13° 02′ 54.0″ | 6.39 | −0.49 | 776 | G8III | |
| 39 Cnc | | 39 | | 73665 | 42516 | 08$^h$ 40$^m$ 06.44$^s$ | +20° 00′ 28.1″ | 6.39 | 0.11 | 587 | K0III | pertany al Cúmul del pessebre; probablement variable |
| HD 78175 | | | | 78175 | 44768 | 09$^h$ 07$^m$ 27.01$^s$ | +22° 58′ 51.1″ | 6.39 | 2.54 | 192 | F5V | |
| X Cnc | | | X | 76221 | 43811 | 08$^h$ 55$^m$ 22.88$^s$ | +17° 13′ 52.5″ | 6.40 | −3.95 | 3622 | C6,4 | variable semiregular, V$_{max}$ = 5.69$^m$, V$_{min}$ = 6.94$^m$, P = 180 d |
| HD 80064 | | | | 80064 | 45614 | 09$^h$ 17$^m$ 51.36$^s$ | +11° 30′ 04.1″ | 6.40 | 0.30 | 542 | A2IV | |
| HD 75469 | | | | 75469 | 43427 | 08$^h$ 50$^m$ 45.13$^s$ | +18° 49′ 56.1″ | 6.41 | −0.43 | 762 | A2Vs | |
| HD 69629 | | | | 69629 | 40675 | 08$^h$ 18$^m$ 14.43$^s$ | +15° 40′ 40.6″ | 6.42 | 0.56 | 485 | K0 | |
| HD 73710 | | | | 73710 | 42549 | 08$^h$ 40$^m$ 22.11$^s$ | +19° 40′ 11.9″ | 6.42 | −0.41 | 756 | K0III | pertany al Cúmul del pessebre |
| ψ¹ Cnc | ψ¹ | 13 | | 67690 | 40007 | 08$^h$ 10$^m$ 13.12$^s$ | +25° 50′ 40.4″ | 6.44 | −1.06 | 1032 | K0 | |
| HD 73599 | | | | 73599 | 42462 | 08$^h$ 39$^m$ 24.57$^s$ | +08° 01′ 03.6″ | 6.46 | 0.32 | 551 | K1III | |
| HD 77660 | | | | 77660 | 44574 | 09$^h$ 04$^m$ 55.12$^s$ | +32° 22′ 37.2″ | 6.46 | 1.96 | 259 | A8V | |
| HD 67542 | | | | 67542 | 39958 | 08$^h$ 09$^m$ 35.19$^s$ | +29° 05′ 35.1″ | 6.47 | −3.93 | 3928 | G0II | |
| HD 68703 | | | | 68703 | 40342 | 08$^h$ 14$^m$ 11.14$^s$ | +17° 40′ 33.3″ | 6.47 | 1.45 | 329 | A0Vne... | |
| HD 78234 | | | | 78234 | 44825 | 09$^h$ 08$^m$ 04.21$^s$ | +32° 32′ 25.6″ | 6.47 | 1.32 | 349 | F2V | |
| 34 Cnc | | 34 | | 72359 | 41904 | 08$^h$ 32$^m$ 39.87$^s$ | +10° 03′ 57.7″ | 6.48 | 0.38 | 541 | A1V | probablement variable |
| HD 78661 | | | | 78661 | 44984 | 09$^h$ 09$^m$ 46.45$^s$ | +11° 33′ 52.3″ | 6.48 | 3.60 | 123 | F2p | probablement variable |
| HD 79248 | | | | 79248 | 45272 | 09$^h$ 13$^m$ 37.27$^s$ | +21° 16′ 59.6″ | 6.48 | 0.57 | 496 | A2V | |
| HD 76908 | | | | 76908 | 44148 | 08$^h$ 59$^m$ 26.89$^s$ | +13° 04′ 27.9″ | 6.49 | −1.50 | 1294 | K5III | |
| 81 Cnc | π¹ | 81 | | 79096 | 45170 | 09$^h$ 12$^m$ 17.87$^s$ | +14° 59′ 43.6″ | 6.49 | 4.93 | 67 | G9V | |
| HD 72115 | | | | 72115 | 41833 | 08$^h$ 31$^m$ 41.31$^s$ | +18° 59′ 16.0″ | 6.50 | −0.99 | 1025 | K0 | |
| 24 Cnc A | | 24 | | 71152 | 41389 | 08$^h$ 26$^m$ 39.82$^s$ | +24° 32′ 03.7″ | 6.51 | 2.11 | 248 | F0III | pertany al sistema 24 Cnc; probablement variable |
| 37 Cnc | | 37 | | 73316 | 42353 | 08$^h$ 38$^m$ 05.19$^s$ | +09° 34′ 28.7″ | 6.54 | 1.25 | 373 | A1V | |
| 35 Cnc | | 35 | | 72779 | 42133 | 08$^h$ 35$^m$ 19.47$^s$ | +19° 35′ 24.3″ | 6.55 | 0.28 | 585 | G0III | |
| ι Cnc B | ι | 48 | | 74738 | 43100 | 08$^h$ 46$^m$ 40.00$^s$ | +28° 45′ 54.6″ | 6.58 | 2.77 | 188 | G8II... | pertany al sistema ι Cnc |
| 40 Cnc | | 40 | | 73666 | 42523 | 08$^h$ 40$^m$ 11.47$^s$ | +19° 58′ 16.2″ | 6.61 | 0.40 | 570 | A1V | pertany al Cúmul del pessebre; endarrerida blava |
| 83 Cnc | | 83 | | 80218 | 45699 | 09$^h$ 18$^m$ 58.91$^s$ | +17° 42′ 20.4″ | 6.61 | 3.64 | 128 | F5 | |
| 38 Cnc | | 38 | BT | 73575 | 42485 | 08$^h$ 39$^m$ 42.68$^s$ | +19° 46′ 42.5″ | 6.66 | 0.59 | 531 | F0III | pertany al Cúmul del pessebre; variable δ Sct, ΔV = 0.06$^m$, P = 0.10 d |
| 70 Cnc | | 70 | | 77557 | 44512 | 09$^h$ 04$^m$ 09.87$^s$ | +27° 53′ 53.9″ | 6.67 | 0.33 | 605 | A1V | |
| 2 LMi | | (2) | | 73427 | 42472 | 08$^h$ 39$^m$ 31.87$^s$ | +32° 30′ 56.2″ | 6.69 | −1.18 | 1220 | K5 | |
| 3 LMi | | (3) | | 73508 | 42503 | 08$^h$ 39$^m$ 56.35$^s$ | +32° 43′ 38.2″ | 6.71 | 0.66 | 528 | K0 | |
| EP Cnc | | | EP | 73819 | 42600 | 08$^h$ 40$^m$ 56.30$^s$ | +19° 34′ 49.2″ | 6.76 | | 556 | A6Vn | pertany al Cúmul del pessebre; variable δ Sct, ΔV = 0.03$^m$ |
| 42 Cnc | | 42 | | 73785 | 42578 | 08$^h$ 40$^m$ 43.23$^s$ | +19° 43′ 09.6″ | 6.83 | 0.87 | 506 | A9III | pertany al Cúmul del pessebre |
| 7 Cnc | | 7 | | 66347 | 39447 | 08$^h$ 03$^m$ 50.48$^s$ | +22° 04′ 14.9″ | 6.84 | | 668 | K0 | |
| 80 Cnc | | 80 | | 79009 | 45153 | 09$^h$ 11$^m$ 56.93$^s$ | +18° 02′ 39.0″ | 6.87 | 1.08 | 470 | A0 | |
| 78 Cnc | | 78 | | 78479 | 44918 | 09$^h$ 09$^m$ 02.31$^s$ | +17° 28′ 10.7″ | 7.18 | | 706 | K3III | |
| VZ Cnc | | | VZ | 73857 | 42594 | 08$^h$ 40$^m$ 52.13$^s$ | +09° 49′ 27.1″ | 7.18 | | 509 | A9III | variable δ Sct, V$_{max}$ = 7.18$^m$, V$_{min}$ = 7.91$^m$, P = 0.18 d |
| ADS 7284 | | | IP | 79969 | 45617 | 09$^h$ 17$^m$ 53.46$^s$ | +28° 33′ 37.9″ | 7.21 | | 56.28 | K3V | variable BY Dra, ΔV = 0.02$^m$, P = 43.4 d |
| 52 Cnc | | 52 | | 75558 | 43463 | 08$^h$ 51$^m$ 10.83$^s$ | +15° 59′ 57.8″ | 7.38 | 1.03 | 607 | G5 | |
| V Cnc | | | V | 70276 | 40977 | 08$^h$ 21$^m$ 42.84$^s$ | +17° 17′ 07.2″ | 7.50 | | | S0-6/6e | variable Mira, V$_{max}$ = 7.5$^m$, V$_{min}$ = 13.9$^m$, P = 270 d |
| T Cnc | | | T | | 43905 | 08$^h$ 56$^m$ 40.15$^s$ | +19° 50′ 57.0″ | 7.60 | | | C | variable semiregular, V$_{max}$ = 7.6$^m$, V$_{min}$ = 10.5$^m$, P = 482 d |
| BU Cnc | | | BU | 73576 | | 08$^h$ 39$^m$ 44.67$^s$ | +19° 16′ 30.8″ | 7.68 | | 577 | A7Vn | pertany al Cúmul del pessebre; variable δ Sct, ΔV = 0.03$^m$, P = 0.071 d |
| BN Cnc | | | BN | 73763 | | 08$^h$ 40$^m$ 39.24$^s$ | +19° 13′ 41.8″ | 7.80 | | 577 | A9V | pertany al Cúmul del pessebre; variable δ Sct, ΔV = 0.03$^m$, P = 0.039 d |
| 24 Cnc B | | 24 | | 71153 | | 08$^h$ 26$^m$ 40.10$^s$ | +24° 32′ 07.0″ | 7.81 | | | | forma part del sistema 24 Cnc |
| BY Cnc | | | BY | 74050 | 42705 | 08$^h$ 42$^m$ 10.81$^s$ | +18° 56′ 03.7″ | 7.91 | | 451 | A7Vn | pertany al Cúmul del pessebre; variable δ Sct, ΔV = 0.01$^m$, P = 0.058 d |
| HD 74028 | | | BX | 74028 | | 08$^h$ 42$^m$ 06.50$^s$ | +19° 24′ 40.5″ | 7.96 | | 577 | A7V | pertany al Cúmul del pessebre; variable δ Sct, ΔV = 0.02$^m$, P = 0.044 d |
| 44 Cnc | | 44 | | 74200 | 42791 | 08$^h$ 43$^m$ 08.36$^s$ | +18° 09′ 02.0″ | 8.03 | | 726 | K0 | |
| HD 79498 | | | | 79498 | 45406 | 09$^h$ 15$^m$ 09$^s$ | +23° 22′ 32″ | 8.03 | | 150 | G5 | té un planeta (b) |
| 71 Cnc | | 71 | | 77802 | 44637 | 09$^h$ 05$^m$ 45.52$^s$ | +17° 23′ 24.5″ | 8.10 | | 672 | A2 | |
| CY Cnc | | | CY | 73345 | | 08$^h$ 38$^m$ 37.86$^s$ | +19° 59′ 23.1″ | 8.14 | | 582 | F0V | pertany al Cúmul del pessebre; variable δ Sct, ΔV = 0.02$^m$, P = 0.1 d |
| BQ Cnc | | | BQ | 73729 | | 08$^h$ 40$^m$ 26.75$^s$ | +20° 10′ 55.2″ | 8.19 | | 577 | F2Vn | pertany al Cúmul del pessebre; variable δ Sct, ΔV = 0.02$^m$, P = 0.074 d |
| HD 73534 | | | | 73534 | 42446 | 08$^h$ 39$^m$ 15.80$^s$ | +12° 57′ 37.3″ | 8.24 | 3.30 | 316 | G5IV | té un planeta (b) |
| BR Cnc | | | BR | 73175 | 42319 | 08$^h$ 37$^m$ 40.71$^s$ | +19° 31′ 06.3″ | 8.26 | | 608 | F0Vn | pertany al Cúmul del pessebre; variable δ Sct, ΔV = 0.02$^m$, P = 0.038 d |
| S Cnc | | | S | 74307 | 42853 | 08$^h$ 43$^m$ 56.14$^s$ | +19° 02′ 03.0″ | 8.35 | | 950 | B9.5V+ G8-9III-IV | variable Algol, V$_{max}$ = 8.29$^m$, V$_{min}$ = 10.25$^m$, P = 9.48 d |
| BW Cnc | | | BW | 73798 | | 08$^h$ 40$^m$ 52.48$^s$ | +20° 15′ 59.5″ | 8.48 | | 577 | F0Vn | pertany al Cúmul del pessebre; variable δ Sct, ΔV = 0.01$^m$, P = 0.072 d |
| TW Cnc | | | TW | 71780 | | 08$^h$ 29$^m$ 37.32$^s$ | +12° 27′ 20.3″ | 8.49 | | | G8III+... | variable Algol, V$_{max}$ = 8.5$^m$, V$_{min}$ = 8.97$^m$, P = 70.76 d |
| U Cnc | | | U | 72863 | | 08$^h$ 35$^m$ 46.29$^s$ | +18° 53′ 44.5″ | 8.50 | | | M2e | variable Mira, V$_{max}$ = 8.5$^m$, V$_{min}$ = 15.5$^m$, P = 306 d |
| BS Cnc | | | BS | 73450 | | 08$^h$ 39$^m$ 09.10$^s$ | +19° 35′ 32.6″ | 8.59 | | 577 | A9V | pertany al Cúmul del pessebre; variable δ Sct, ΔV = 0.02$^m$, P = 0.051 d |
| R Cnc | | | R | 69243 | 40534 | 08$^h$ 16$^m$ 33.90$^s$ | +11° 43′ 35.0″ | 8.64 | | 2060 | M6.5-9e | variable Mira, V$_{max}$ = 6.07$^m$, V$_{min}$ = 11.9$^m$, P = 357 d |
| BV Cnc | | | BV | 73746 | | 08$^h$ 40$^m$ 32.97$^s$ | +19° 11′ 39.6″ | 8.65 | | 577 | F0V | pertany al Cúmul del pessebre; variable δ Sct, ΔV = 0.02$^m$, P = 0.21 d |
| RZ Cnc | | | RZ | 73343 | 42432 | 08$^h$ 39$^m$ 08.54$^s$ | +31° 47′ 44.4″ | 8.67 | | 1420 | K2III | variable RS CVn, V$_{max}$ = 8.67$^m$, V$_{min}$ = 10.03$^m$, P = 21.64 d |
| HD 74721 | | | | 74721 | 43018 | 08$^h$ 45$^m$ 59.26$^s$ | +13° 15′ 48.6″ | 8.72 | | | A0V | estrella branca horitzontal |
| UU Cnc | | | UU | | 39341 | 08$^h$ 02$^m$ 30.90$^s$ | +15° 10′ 41.9″ | 8.85 | | | K4III... | variable β Lyr, V$_{max}$ = 8.68$^m$, V$_{min}$ = 9.35$^m$, P = 96.71 d |
| RX Cnc | | | RX | 68775 | 40388 | 08$^h$ 14$^m$ 43.54$^s$ | +24° 44′ 05.3″ | 9.20 | | 931 | M8 | variable semiregular |
| WY Cnc | | | WY | | 44349 | 09$^h$ 01$^m$ 55.45$^s$ | +26° 41′ 22.7″ | 9.60 | | 264.6 | G5V | variable RS CVn, V$_{max}$ = 9.51$^m$, V$_{min}$ = 10.14$^m$, P = 0.83 d |
| TX Cnc | | | TX | | | 08$^h$ 40$^m$ 01.70$^s$ | +18° 59′ 59.5″ | 9.97 | | 626 | G0-G1V | pertany al Cúmul del pessebre; variable W UMa, V$_{max}$ = 10$^m$, V$_{min}$ = 10.35$^m$, P = 0.38 d |
| RU Cnc | | | RU | | 42303 | 08$^h$ 37$^m$ 30.13$^s$ | +23° 33′ 41.6″ | 10.20 | | 911 | F9V:+... | variable RS CVn, V$_{max}$ = 10.1$^m$, V$_{min}$ = 11.25$^m$, P = 10.17 d |
| TU Cnc | | | TU | | | 08$^h$ 52$^m$ 16.65$^s$ | +09° 05′ 18.8″ | 10.53 | | | A2 | variable Algol |
| SY Cnc | | | SY | | | 09$^h$ 01$^m$ 03.32$^s$ | +17° 53′ 56.2″ | 10.60 | | | G8V | variable Z Cam |
| EX Cnc | | | EX | | | 08$^h$ 51$^m$ 34.32$^s$ | +11° 51′ 10.5″ | 10.95 | | 2720 | A7 | en Messier 67; variable δ Sct, ΔV = 0.05$^m$, P = 0.049 d |
| TT Cnc | | | TT | | 41936 | 08$^h$ 32$^m$ 55.18$^s$ | +13° 11′ 28.5″ | 11.10 | | | F0 | variable RR Lyr, V$_{max}$ = 10.93$^m$, V$_{min}$ = 11.57$^m$, P = 0.56 d |
| ES Cnc | | | ES | | | 08$^h$ 51$^m$ 20.79$^s$ | +11° 53′ 26.2″ | 11.16 | | 2720 | F4 | en Messier 67; variable RS CVn, V$_{max}$ = 11.16$^m$, V$_{min}$ = 11.28$^m$, P = 1.07 d |
| HAT-P-31 | | | | | | 08$^h$ 06$^m$ 09$^s$ | +26° 25′ 36″ | 11.66 | | 1155 | | té un planeta en trànsit (b) |
| CU Cnc | | | CU | | 41824 | 08$^h$ 31$^m$ 37.57$^s$ | +19° 23′ 39.4″ | 11.80 | | 36.07 | M5Ve | variable Algol i estrella fulgurant, V$_{max}$ = 11.68$^m$, V$_{min}$ = 11.80$^m$, P = 2.77 d |
| WASP-65 | | | | | | 08$^h$ 53$^m$ 18.0$^s$ | +08° 31′ 23″ | 11.9 | | 1011 | G6 | té un planeta en trànsit (b) |
| SS Cnc | | | SS | | | 08$^h$ 06$^m$ 25.60$^s$ | +23° 15′ 05.7″ | 12.11 | | | A8.5 | variable RR Lyr, V$_{max}$ = 11.49$^m$, V$_{min}$ = 12.72$^m$, P = 0.37 d |
| EW Cnc | | | EW | | | 08$^h$ 51$^m$ 32.58$^s$ | +11° 50′ 40.6″ | 12.27 | | 2720 | F0 | in Messier 67; δ Sct variable, ΔV = 0.02$^m$, P = 0.053 d |
| HV Cnc | | | HV | | | 08$^h$ 51$^m$ 17.99$^s$ | +11° 45′ 54.2″ | 12.73 | | 2720 | | en Messier 67; variable Algol |
| EV Cnc | | | EV | | | 08$^h$ 51$^m$ 28.15$^s$ | +11° 49′ 27.5″ | 12.78 | | 2720 | F3 | en Messier 67; variable W UMa, ΔV = 0.13$^m$, P = 0.44 d |
| AD Cnc | | | AD | | | 08$^h$ 46$^m$ 20.10$^s$ | +10° 20′ 07.2″ | 13.10 | | | K0V | variable W UMa, V$_{max}$ = 13.1$^m$, V$_{min}$ = 13.4$^m$, P = 0.28 d |
| HAT-P-43 | | | | | | 08$^h$ 35$^m$ 42.0$^s$ | +10° 12′ 24″ | 13.36 | | 1771 | | té un planeta en trànsit (b) |
| AH Cnc | | | AH | | | 08$^h$ 51$^m$ 37.85$^s$ | +11° 50′ 57.1″ | 13.41 | | 2720 | F7V | en Messier 67; variable W UMa, V$_{max}$ = 13.31$^m$, V$_{min}$ = 13.96$^m$, P = 0.36 d |
| HU Cnc | | | HU | | | 08$^h$ 51$^m$ 13.36$^s$ | +11° 51′ 40.1″ | 13.61 | | 2720 | G8IV | en Messier 67; variable RS CVn, V$_{max}$ = 13.45$^m$, V$_{min}$ = 13.61$^m$, P = 18.39 d |
| AC Cnc | | | AC | | | 08$^h$ 44$^m$ 27.11$^s$ | +12° 52′ 31.9″ | 13.80 | | | K1-3V | variable Algol, V$_{max}$ = 13.8$^m$, V$_{min}$ = 15.4$^m$, P = 0.30 d |
| G 9-38 | | | EI | | | 08$^h$ 58$^m$ 15.19$^s$ | +19° 45′ 47.1″ | | | 17.2 | M5.5V | estrella fulgurant |
| YBP 1194 | | | | | | 08$^h$ 51$^m$ 00.81$^s$ | +11° 48′ 52.8″ | 14.61 | | 2720 | G5V | en Messier 67; anàleg solar; té tres planetes (b, c i d) |
| DX Cnc | | | DX | | | 08$^h$ 29$^m$ 49.35$^s$ | +26° 46′ 33.7″ | 14.81 | | 11.82 | M6.5V | estrella fulgurant |
| AT Cnc | | | AT | | | 08$^h$ 28$^m$ 36.93$^s$ | +25° 20′ 03.0″ | 15.2 | | | DAe... | variable Z Cam, V$_{max}$ = 12.57$^m$, V$_{min}$ = 15.2$^m$, P = 0.20 d |
| LHS 2090 | | | | | | 09$^h$ 00$^m$ 23.59$^s$ | +21° 50′ 05.4″ | 16.10 | | 20.782 | M6.5V | |
| YZ Cnc | | | YZ | | | 08$^h$ 10$^m$ 56.65$^s$ | +28° 08′ 33.5″ | 16.3 | | | | variable SU UMa, V$_{max}$ = 10.5$^m$, V$_{min}$ = 16.3$^m$, P = 0.087 d |
| EG Cnc | | | EG | | | 08$^h$ 43$^m$ 03.99$^s$ | +27° 51′ 49.7″ | 17.0 | | | | variable WZ Sge, V$_{max}$ = 11.9$^m$, V$_{min}$ = 17.0$^m$, P = 0.060 d |
| DW Cnc | | | DW | | | 07$^h$ 58$^m$ 53.05$^s$ | +16° 16′ 45.2″ | 17.5 | | | O... | nova nana, V$_{max}$ = 11.36$^m$, V$_{min}$ = 17.5$^m$, P = 0.0060 d |
| AZ Cnc | | | AZ | | | 08$^h$ 40$^m$ 29.75$^s$ | +18° 14′ 09.2″ | 17.59 | | 45.7 | M6.0V | estrella fulgurant |
| GY Cnc | | | GY | | | 09$^h$ 09$^m$ 50.55$^s$ | +18° 49′ 47.5″ | 17.8 | | | | nova nana i binària eclipsant, V$_{max}$ = 12.5$^m$, V$_{min}$ = 17.8$^m$, P = 0.18 d |
| AR Cnc | | | AR | | | 09$^h$ 22$^m$ 07.55$^s$ | +31° 03′ 14.5″ | 18.7 | | | | nana nova i variable Algol, V$_{max}$ = 15.3$^m$, V$_{min}$ = 18.7$^m$, P = 0.21 d |
| RX J0806.3+1527 | | | HM | | | 08$^h$ 06$^m$ 22.95$^s$ | +15° 27′ 31.1″ | | | 160 | | estrella AM Canum Venaticorum |
| AK Cnc | | | AK | | | 08$^h$ 55$^m$ 21.18$^s$ | +11° 18′ 15.3″ | | | | | variable SU UMa |
| CC Cnc | | | CC | | | 08$^h$ 36$^m$ 19.15$^s$ | +21° 21′ 05.3″ | | | | K0V | variable SU UMa |
| PSR B0823+26 | | | | | | 08$^h$ 26$^m$ 51.44$^s$ | +26° 37′ 22.8″ | | | | | púlsar |

## Vegeu també

* Llista d'estrelles per constel·lació

## Referències

* ESA. «The Hipparcos and Tycho Catalogues», 1997. [Consulta: 27 desembre 2014].
* Kostjuk, N. D. «HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index», 2002. [Consulta: 27 desembre 2014].
* Roman, N. G. «Identification of a Constellation from a Position», 1987. [Consulta: 27 desembre 2014].
* «SIMBAD Astronomical Database». Centre de Données astronomiques de Strasbourg. [Consulta: 27 desembre 2014].
* Gould, B. A. «Uranometria Argentina». Reprinted and updated by Pilcher, F. Arxivat de l'original el 2012-02-27. [Consulta: 27 desembre 2014].
* Samus, N. N.; Durlevich, O. V.; et al.. «Combined General Catalogue of Variable Stars (GCVS4.2)», 2004. [Consulta: 27 desembre 2014].
* Samus, N. N.; Durlevich, O. V.; et al.. «General Catalog of Variable Stars (GCVS database, version 2012Feb)», 2012. [Consulta: 27 desembre 2014].