The Pavo constellation is formed by 7 main stars. There are currently 104 discovered stars in the region inside its perimeter. Pavo can only be seen in the southern hemisphere.
The constellation of Pavo represents a peacock.
Below you will find the full list of stars in the Pavo constellation and their names as well as some general information about each of them.
Here’s what each of the columns means.
Proper name: This is the common name we give to some of the most prominent stars in the sky. These names have been passed from ancient civilizations and they are usually of Greek or Arabic origin. Due to the number of stars in the universe, most stars discovered these days do not receive a proper name.
Name: The scientific, Latinized name for the star.
Designation: Abbreviation of the scientific name or designation if it doesn’t have one. It is based on the Bayer catalog of stars.
Distance: How far away from Earth the star is. Given in light-years.
Visible magnitude: The brightness of the star as seen from Earth. Also known as apparent magnitude.
Absolute magnitude: The true brightness of the star, regardless of the point of view.
Stellar classification: Classification of the star according to its electromagnetic characteristics.
Proper Name | Name | Designation | Distance (light-years) | Visible magnitude | Absolute magnitude | Stellar classification |
---|---|---|---|---|---|---|
Peacock | Alpha Pavonis | α Pav | 183.00 | 1.94 | −1.81 | B2IV |
Beta Pavonis | β Pav | 137.00 | 3.42 | 0.29 | A5IV | |
Delta Pavonis | δ Pav | 20.00 | 3.55 | 4.62 | G5IV-Vvar | |
Eta Pavonis | η Pav | 371.00 | 3.61 | −1.67 | K1III | |
Epsilon Pavonis | ε Pav | 106.00 | 3.97 | 1.41 | A0V | |
Zeta Pavonis | ζ Pav | 210.00 | 4.01 | −0.03 | K2III | |
Gamma Pavonis | γ Pav | 30.00 | 4.21 | 4.39 | F6V | |
Lambda Pavonis | λ Pav | 1811.00 | 4.22 | −4.50 | B2II-III | |
Pi Pavonis | π Pav | 138.00 | 4.33 | 1.19 | Am | |
Xi Pavonis | ξ Pav | 420.00 | 4.35 | −1.20 | M1III SB | |
Kappa Pavonis | κ Pav | 543.00 | 4.40 | −1.71 | F5Ib-II: | |
Nu Pavonis | ν Pav | 479.00 | 4.63 | −1.20 | B8III | |
Phi1 Pavonis | φ1 Pav | 90.00 | 4.75 | 2.55 | F1III | |
HD 172555 | HD 172555 | 95.00 | 4.78 | 2.45 | A7V | |
Rho Pavonis | ρ Pav | 195.00 | 4.85 | 0.98 | Fm… | |
NU Pavonis | NU Pav | 434.00 | 4.95 | −0.67 | M6III | |
Omicron Pavonis | ο Pav | 888.00 | 5.06 | −2.12 | M2III | |
Phi2 Pavonis | φ2 Pav | 79.00 | 5.11 | 3.19 | F8V | |
Omega Pavonis | ω Pav | 516.00 | 5.14 | −0.86 | K1III-IV | |
Upsilon Pavonis | υ Pav | 840.00 | 5.14 | −1.92 | B8Vvar | |
HD 188162 | HD 188162 | 302.00 | 5.24 | 0.41 | B9.5IV | |
HD 177389 | HD 177389 | 120.00 | 5.31 | 2.48 | G8/K0III/IV | |
Mu2 Pavonis | μ2 Pav | 234.00 | 5.32 | 1.04 | K2IVCN… | |
HD 186219 | HD 186219 | 135.00 | 5.39 | 2.3 | A4III | |
HD 186957 | HD 186957 | 260.00 | 5.41 | 0.9 | A0IV | |
Sigma Pavonis | σ Pav | 305.00 | 5.41 | 0.56 | K0III | |
Iota Pavonis | ι Pav | 58.00 | 5.47 | 4.22 | G0V | |
SX Pavonis | SX Pav | 396.00 | 5.47 | 0.05 | M5III | |
HD 179366 | HD 179366 | 296.00 | 5.52 | 0.73 | A4IV/V | |
HD 166599 | HD 166599 | 296.00 | 5.58 | 0.79 | K0III/IV | |
HD 198160 | HD 198160 | 238.00 | 5.67 | 1.35 | A2 | |
HD 200525 | HD 200525 | 61.00 | 5.67 | 4.31 | G3IV | |
Theta Pavonis | θ Pav | 226.00 | 5.71 | 1.51 | A9V | |
HD 169836 | HD 169836 | 357.00 | 5.74 | 0.54 | K0III | |
HD 188097 | HD 188097 | 232.00 | 5.74 | 1.48 | Am | |
Mu1 Pavonis | μ1 Pav | 216.00 | 5.75 | 1.64 | K0IV | |
HD 200751 | HD 200751 | 489.00 | 5.75 | −0.13 | K0III | |
HD 172211 | HD 172211 | 410.00 | 5.76 | 0.26 | K0III | |
HD 161814 | HD 161814 | 371.00 | 5.78 | 0.5 | K0III | |
HD 169570 | HD 169570 | 356.00 | 5.88 | 0.69 | K0III | |
HD 175986 | HD 175986 | 185.00 | 5.89 | 2.12 | F8V | |
HD 160720 | HD 160720 | 406.00 | 5.97 | 0.49 | G8III | |
HD 175401 | HD 175401 | 439.00 | 5.98 | 0.33 | K0III | |
HD 182709 | HD 182709 | 1042.00 | 5.98 | −1.54 | K4/K5III | |
HD 172630 | HD 172630 | 1035.00 | 6.04 | −1.47 | K3III | |
HD 172881 | HD 172881 | 736.00 | 6.04 | −0.73 | B9.5IV/V | |
NZ Pavonis | NZ Pav | 196.00 | 6.04 | 2.15 | F2III-IV | |
HD 189567 | HD 189567 | 58.00 | 6.07 | 4.83 | G2V | |
HD 184996 | HD 184996 | 753.00 | 6.08 | −0.74 | M0III | |
HD 191603 | HD 191603 | 235.00 | 6.09 | 1.8 | F0IV | |
HD 195402 | HD 195402 | 830.00 | 6.09 | −0.94 | K2III | |
HD 203212 | HD 203212 | 531.00 | 6.09 | 0.03 | K2III | |
HD 168740 | HD 168740 | 232.00 | 6.13 | 1.87 | A3V | |
HD 167425 | HD 167425 | 75.00 | 6.17 | 4.37 | F9V | |
HD 200924 | HD 200924 | 390.00 | 6.18 | 0.79 | K1III | |
HD 184585 | HD 184585 | 482.00 | 6.19 | 0.34 | K0III | |
HD 186837 | HD 186837 | 898.00 | 6.21 | −0.99 | B5V | |
HD 187653 | HD 187653 | 304.00 | 6.21 | 1.36 | A3V | |
HD 172781 | HD 172781 | 685.00 | 6.22 | −0.39 | K3III | |
HD 196317 | HD 196317 | 426.00 | 6.22 | 0.64 | K1III | |
Tau Pavonis | τ Pav | 619.00 | 6.25 | −0.14 | A6IV/V | |
HD 192531 | HD 192531 | 445.00 | 6.27 | 0.59 | K0III | |
Y Pavonis | Y Pav | 1181.00 | 6.28 | −1.52 | C5II | |
HD 176522 | HD 176522 | 565.00 | 6.30 | 0.11 | G6II/III | |
HD 166841 | HD 166841 | 697.00 | 6.32 | −0.33 | B9V | |
HD 202299 | HD 202299 | 552.00 | 6.32 | 0.18 | B8V | |
HD 181019 | HD 181019 | 676.00 | 6.33 | −0.25 | K2III | |
HD 195772 | HD 195772 | 191.00 | 6.34 | 2.5 | F2V | |
HD 172021 | HD 172021 | 767.00 | 6.35 | −0.51 | A5V | |
HD 162521 | HD 162521 | 113.00 | 6.36 | 3.67 | F8V | |
HD 191095 | HD 191095 | 452.00 | 6.36 | 0.65 | A1V | |
HD 199475 | HD 199475 | 272.00 | 6.36 | 1.76 | A2V | |
HD 184586 | HD 184586 | 335.00 | 6.37 | 1.31 | A0Vn | |
HD 165497 | HD 165497 | 642.00 | 6.38 | −0.09 | K4III | |
HD 188164 | HD 188164 | 341.00 | 6.38 | 1.28 | A2V | |
HD 164871 | HD 164871 | 535.00 | 6.40 | 0.32 | K2/K3III | |
HD 170525 | HD 170525 | 164.00 | 6.40 | 2.89 | G5IV | |
HD 161475 | HD 161475 | 689.00 | 6.41 | −0.22 | B9IV | |
HD 195190 | HD 195190 | 805.00 | 6.41 | −0.55 | K2III | |
HD 179419 | HD 179419 | 700.00 | 6.42 | −0.24 | B8/B9V | |
HD 186584 | HD 186584 | 1076.00 | 6.44 | −1.15 | K4III | |
HD 190222 | HD 190222 | 1144.00 | 6.45 | −1.28 | K5III | |
HD 166251 | HD 166251 | 614.00 | 6.47 | 0.1 | K4III | |
HD 174877 | HD 174877 | 1136.00 | 6.47 | −1.24 | K3III | |
HD 161955 | HD 161955 | 519.00 | 6.48 | 0.47 | K0/K1III | |
HD 175007 | HD 175007 | 351.00 | 6.49 | 1.33 | A8V | |
HD 192887 | HD 192887 | 143.00 | 6.49 | 3.27 | F6V | |
V Pavonis | V Pav | 1210.00 | 6.84 | C+ | ||
HD 164427 | HD 164427 | 123.90 | 6.84 | G0+V | ||
AR Pavonis | AR Pav | 2300.00 | 7.40 | B1 | ||
R Pavonis | R Pav | 1100.00 | 7.50 | M4.5e | ||
HD 196050 | HD 196050 | 153.00 | 7.60 | 4.2 | G3V | |
KZ Pavonis | KZ Pav | 434.00 | 7.71 | F6V | ||
HD 175167 | HD 175167 | 219.00 | 8.00 | 3.87 | G5IV/V | |
HD 181433 | HD 181433 | 87.00 | 8.38 | 6.24 | K5V | |
HD 175607 | HD 175607 | 148.00 | 8.60 | G6V | ||
HD 190984 | HD 190984 | 618.00 | 8.73 | 2.34 | F8V | |
MW Pavonis | MW Pav | 682.00 | 8.79 | F3IV/V | ||
X Pavonis | X Pav | 2190.00 | 9.20 | M6/M7III:p | ||
Gliese 693 | Gliese 693 | 19.01 | 10.78 | M2.0 | ||
V347 Pavonis | V347 Pav | 14.85 | CV | |||
SCR 1845-6357 | SCR 1845-6357 | 12.56 | 17.40 | M8.5 | ||
BD Pavonis | BD Pav |