# List of stars in Corona Australis

This is the list of notable stars in the constellation Corona Australis, sorted by decreasing brightness.
| Name | B | Var | HD | HIP | RA | Dec | vis. mag. | abs. mag. | Dist. (ly) | Sp. class | Notes |
| β CrA | β | | 178345 | 94160 | 19$^h$ 10$^m$ 01.75$^s$ | −39° 20′ 26.5″ | 4.10 | −1.86 | 508 | K0II/IIICN. | suspected variable |
| α CrA | α | | 178253 | 94114 | 19$^h$ 09$^m$ 28.28$^s$ | −37° 54′ 15.3″ | 4.11 | 1.11 | 130 | A0/A1V | Meridiana (traditionally Alphekka Meridiana, Alfecca Meridiana) |
| γ CrA A | γ | | 177474 | 93825 | 19$^h$ 06$^m$ 25.04$^s$ | −37° 03′ 45.9″ | 4.23 | 2.97 | 58 | F7IV-V | double star |
| δ CrA | δ | | 177873 | 94005 | 19$^h$ 08$^m$ 20.93$^s$ | −40° 29′ 47.9″ | 4.57 | 0.93 | 175 | K1III | |
| θ CrA | θ | | 170845 | 90982 | 18$^h$ 33$^m$ 30.16$^s$ | −42° 18′ 44.9″ | 4.62 | −2.50 | 867 | G5III | |
| ζ CrA | ζ | | 176638 | 93542 | 19$^h$ 03$^m$ 06.83$^s$ | −42° 05′ 42.0″ | 4.74 | 0.99 | 184 | A0Vn | |
| ε CrA | ε | | 175813 | 93174 | 18$^h$ 58$^m$ 43.47$^s$ | −37° 06′ 25.5″ | 4.83 | 2.45 | 98 | F3IV/V | W UMa variable, V$_{max}$ = 4.74$^m$, V$_{min}$ = 5$^m$, P = 0.5914264 d |
| HD 165189 | | | 165189 | 88726 | 18$^h$ 06$^m$ 49.88$^s$ | −43° 25′ 29.9″ | 4.92 | 1.71 | 143 | A5V | |
| γ CrA B | γ | | 177475 | | 19$^h$ 06$^m$ 25.10$^s$ | −37° 03′ 48.0″ | 4.99 | | | | component of the γ CrA system |
| HD 168592 | | | 168592 | 90037 | 18$^h$ 22$^m$ 18.60$^s$ | −38° 39′ 24.6″ | 5.09 | −0.85 | 503 | K4/K5III | |
| λ CrA | λ | | 172777 | 91875 | 18$^h$ 43$^m$ 46.94$^s$ | −38° 19′ 23.9″ | 5.11 | 1.15 | 202 | A0/A1V | suspected variable, ΔV = 0.07$^m$ |
| HD 170642 | | | 170642 | 90887 | 18$^h$ 32$^m$ 21.31$^s$ | −39° 42′ 14.1″ | 5.16 | 1.02 | 220 | A3V | |
| μ CrA | μ | | 173540 | 92226 | 18$^h$ 47$^m$ 44.60$^s$ | −40° 24′ 22.0″ | 5.20 | −0.20 | 393 | G5/G6III | |
| HD 168905 | | | 168905 | 90200 | 18$^h$ 24$^m$ 18.24$^s$ | −44° 06′ 36.7″ | 5.24 | −0.79 | 524 | B2.5Vn | suspected variable |
| HD 175219 | | | 175219 | 92953 | 18$^h$ 56$^m$ 16.97$^s$ | −42° 42′ 38.2″ | 5.35 | 0.46 | 310 | G6III-IV | |
| V686 CrA | | V686 | 175362 | 92989 | 18$^h$ 56$^m$ 40.49$^s$ | −37° 20′ 35.5″ | 5.36 | −0.22 | 425 | B3V | α$^2$ CVn variable, V$_{max}$ = 5.25$^m$, V$_{min}$ = 5.41$^m$, P = 7.34 d |
| HD 172991 | | | 172991 | 91989 | 18$^h$ 44$^m$ 57.15$^s$ | −39° 41′ 10.2″ | 5.40 | −2.64 | 1320 | K1/K2III+.. | |
| V718 CrA | | V718 | 171967 | 91494 | 18$^h$ 39$^m$ 35.18$^s$ | −43° 11′ 08.8″ | 5.42 | −1.58 | 817 | M2III | slow irregular variable |
| HD 167096 | | | 167096 | 89507 | 18$^h$ 15$^m$ 53.39$^s$ | −44° 12′ 23.4″ | 5.45 | 0.87 | 268 | G8/K0III | |
| η$^1$ CrA | η$^1$ | | 173715 | 92308 | 18$^h$ 48$^m$ 50.47$^s$ | −43° 40′ 48.0″ | 5.46 | 0.33 | 347 | A2Vn | |
| V692 CrA | | V692 | 166596 | 89290 | 18$^h$ 13$^m$ 12.70$^s$ | −41° 20′ 09.9″ | 5.47 | −3.06 | 1655 | B2.5III | SX Ari variable, ΔV = 0.05$^m$, P = 1.67 d |
| η$^2$ CrA | η$^2$ | | 173861 | 92382 | 18$^h$ 49$^m$ 35.00$^s$ | −43° 26′ 02.5″ | 5.60 | −0.75 | 607 | B9IV | |
| HD 169853 | | | 169853 | 90541 | 18$^h$ 28$^m$ 27.11$^s$ | −38° 59′ 44.1″ | 5.63 | −0.29 | 498 | A2m... | |
| κ$^2$ CrA | κ$^2$ | | 170868 | 90968 | 18$^h$ 33$^m$ 23.13$^s$ | −38° 43′ 33.4″ | 5.67 | −2.94 | 1716 | B9.5 | |
| HD 170521 | | | 170521 | 90842 | 18$^h$ 31$^m$ 56.22$^s$ | −43° 30′ 26.5″ | 5.71 | −2.20 | 1244 | K2III | |
| V701 CrA | | V701 | 176723 | 93552 | 19$^h$ 03$^m$ 17.69$^s$ | −38° 15′ 11.5″ | 5.73 | 1.68 | 211 | F2III/IV | δ Sct variable, V$_{max}$ = 5.69$^m$, V$_{min}$ = 5.73$^m$ |
| HD 166114 | | | 166114 | 89099 | 18$^h$ 11$^m$ 05.54$^s$ | −41° 21′ 32.5″ | 5.86 | 1.28 | 269 | F0Vn | suspected variable |
| HD 178322 | | | 178322 | 94157 | 19$^h$ 09$^m$ 57.65$^s$ | −41° 53′ 32.0″ | 5.86 | −1.14 | 817 | B5V | suspected variable |
| HD 179433 | | | 179433 | 94556 | 19$^h$ 14$^m$ 39.52$^s$ | −45° 11′ 36.4″ | 5.91 | 1.12 | 296 | G8III | |
| HD 170384 | | | 170384 | 90759 | 18$^h$ 31$^m$ 02.95$^s$ | −41° 54′ 49.5″ | 6.02 | 1.55 | 255 | A3V | |
| HD 177565 | | | 177565 | 93858 | 19$^h$ 06$^m$ 52.60$^s$ | −37° 48′ 35.2″ | 6.15 | 4.98 | 56 | G8V | has a planet (b) |
| HD 176425 | | | 176425 | 93470 | 19$^h$ 02$^m$ 08.50$^s$ | −41° 54′ 37.7″ | 6.21 | 1.04 | 352 | A0V | |
| HD 170773 | | | 170773 | 90936 | 18$^h$ 33$^m$ 00.85$^s$ | −39° 53′ 30.6″ | 6.22 | 3.43 | 118 | F5V | |
| HD 175395 | | | 175395 | 93049 | 18$^h$ 57$^m$ 14.31$^s$ | −43° 55′ 01.0″ | 6.27 | −0.43 | 712 | B9V | |
| HD 175529 | | | 175529 | 93074 | 18$^h$ 57$^m$ 34.39$^s$ | −39° 49′ 23.8″ | 6.29 | 2.34 | 201 | A5IV/V | |
| HD 167756 | | | 167756 | 89726 | 18$^h$ 18$^m$ 40.15$^s$ | −42° 17′ 18.2″ | 6.30 | | | B0.5Ia | suspected variable, ΔV = 0.03$^m$ |
| κ$^1$ CrA | κ$^1$ | | 170867 | 90969 | 18$^h$ 33$^m$ 23.08$^s$ | −38° 43′ 12.0″ | 6.31 | 0.43 | 489 | B8 | |
| HD 178628 | | | 178628 | 94243 | 19$^h$ 11$^m$ 01.91$^s$ | −39° 00′ 16.9″ | 6.34 | −3.19 | 2629 | B7II/III | |
| HD 169943 | | | 169943 | 90597 | 18$^h$ 29$^m$ 12.87$^s$ | −43° 50′ 45.6″ | 6.36 | 0.38 | 512 | G8III | |
| HD 176270 | | | 176270 | 93371 | 19$^h$ 01$^m$ 04.30$^s$ | −37° 03′ 41.4″ | 6.44 | 2.00 | 252 | B9.5IV: | |
| HD 178254 | | | 178254 | 94130 | 19$^h$ 09$^m$ 39.76$^s$ | −39° 49′ 37.9″ | 6.44 | 1.29 | 350 | K0III | |
| HD 168357 | | | 168357 | 89920 | 18$^h$ 20$^m$ 55.19$^s$ | −37° 29′ 15.5″ | 6.46 | −2.76 | 2280 | K2II | |
| HD 174407 | | | 174407 | 92608 | 18$^h$ 52$^m$ 11.95$^s$ | −41° 42′ 32.8″ | 6.47 | −0.13 | 682 | K3III | |
| HD 175093 | | | 175093 | 92866 | 18$^h$ 55$^m$ 23.55$^s$ | −37° 23′ 11.8″ | 6.48 | 0.91 | 424 | K1III | |
| HD 175855 | | | 175855 | 93209 | 18$^h$ 59$^m$ 10.97$^s$ | −39° 32′ 04.7″ | 6.49 | 0.62 | 486 | B9.5V | |
| HD 174152 | | | 174152 | 92487 | 18$^h$ 50$^m$ 58.65$^s$ | −41° 03′ 45.6″ | 6.50 | −2.18 | 1772 | B5III | |
| V693 CrA | | V693 | | | 18$^h$ 41$^m$ 57.8$^s$ | −37° 31′ 14″ | 6.50 | | | | nova, V$_{max}$ = 6.5$^m$, V$_{min}$ = <19.0$^m$ |
| V394 CrA | | V394 | | | 18$^h$ 00$^m$ 25.97$^s$ | −39° 00′ 35.1″ | 7.50 | | | | recurrent nova and eclipsing binary, V$_{max}$ = 7.2$^m$, V$_{min}$ = 19.7$^m$, P = 1.515682 d |
| HD 166473 | | V694 | 166473 | | 18$^h$ 12$^m$ 25.83$^s$ | −37° 45′ 09.2″ | 7.92 | | | A5p | rapidly oscillating Ap star and α$^2$ CVn variable |
| HD 166724 | | | 166724 | 89354 | 18$^h$ 14$^m$ 00$^s$ | −42° 34′ 31″ | 9.31 | | 138 | K0IV | has a planet (b) |
| TY CrA | | TY | | | 19$^h$ 01$^m$ 40.83$^s$ | −36° 52′ 33.9″ | 9.39 | | | B8e | Orion and Algol variable, V$_{max}$ = 9.39$^m$, V$_{min}$ = 9.81$^m$, P = 2.8877912 d |
| V CrA | | V | 173539 | 92207 | 18$^h$ 47$^m$ 32.31$^s$ | −38° 09′ 32.3″ | 9.40 | | | R... | R Coronae Borealis variable, V$_{max}$ = 9.4$^m$, V$_{min}$ = 17.9$^m$ |
| S CrA | | S | | | 19$^h$ 01$^m$ 08.60$^s$ | −36° 57′ 20.0″ | 10.49 | | | G0Ve+K0Ve | Orion variable in nebula, V$_{max}$ = 10.49$^m$, V$_{min}$ = 13.2$^m$ |
| R CrA | | R | | 93449 | 19$^h$ 01$^m$ 53.65$^s$ | −36° 57′ 07.6″ | 11.50 | | 79.64 | A5IIev | Orion variable in nebula |
| T CrA | | T | | | 19$^h$ 01$^m$ 58.78$^s$ | −36° 57′ 49.9″ | 11.67 | | | F0e | Orion variable in nebula, V$_{max}$ = 11.67$^m$, V$_{min}$ = 14.3$^m$ |
| 2A 1822-371 | | V691 | | | 18$^h$ 25$^m$ 46.81$^s$ | −37° 06′ 18.6″ | 15.10 | | | | Low-mass X-ray binary (pulsar) and eclipsing binary |
| RX J1856.5-3754 | | | | | 18$^h$ 56$^m$ 35.11$^s$ | −37° 54′ 30.5″ | 25.7 | | 400 | | closest known neutron star to Earth; possible quark star |
| Y CrA | | Y | 166813 | | 18$^h$ 14$^m$ 22.95$^s$ | −42° 50′ 32.4″ | | | | M6 | Z Andromedae variable |
| RU CrA | | RU | 180206 | | 19$^h$ 17$^m$ 23.46$^s$ | −39° 36′ 46.40″ | | | | [WC3/4] | slow irregular variable; central star of planetary nebula IC 1297 |
| Table legend:  • Name = Proper name  • B = Bayer designation  • F or/and G. = Flamsteed designation or Gould designation  • Var = Variable star designation  • HD = Henry Draper Catalogue designation number  • HIP = Hipparcos Catalogue designation number  • RA = Right ascension for the Epoch/Equinox J2000.0  • Dec = Declination for the Epoch/Equinox J2000.0  • vis. mag. = visual magnitude (m or m$_v$), also known as apparent magnitude  • abs. mag. = absolute magnitude (M$_v$)  • Dist. (ly) = Distance in light-years from Earth  • Sp. class = Spectral class of the star in the stellar classification system  • Notes = Common name(s) or alternate name(s); comments; notable properties [for example: multiple star status, range of variability if it is a variable star, exoplanets, etc.] ||||||||||||