List of brightest stars facts for kids
This article lists stars based on their apparent magnitude. This is how bright they appear to us from Earth. It's different from how truly bright a star is, which is called its absolute magnitude. Many stars look bright because they are close to us, not because they are super powerful.
The brightness of stars is measured using a special scale called the magnitude scale. On this scale, smaller numbers mean a star is brighter. Even negative numbers are possible for the very brightest objects! For example, the Sun has a very low (negative) magnitude because it's so bright to us.
Contents
How We Measure Star Brightness
The Sun is by far the brightest star we see from Earth, with a magnitude of about -26.74. The next brightest star is Sirius, at about -1.46.
To give you an idea, here are some other bright objects in our Solar System and their brightest magnitudes:
It's not always easy to rank stars perfectly by how bright they look. Here's why:
Stars in Groups
Sometimes, what looks like one star is actually two or more stars very close together. These are called binary stars or multiple star systems.
- If they look like a single point of light to our eyes, we measure their total brightness.
- If you can see them as separate stars, they are listed individually.
For example, Alpha Centauri looks like one bright star, but it's actually two main stars. Their combined brightness is -0.27, but their individual brightnesses are +0.01 and +1.33.
Different Ways to Measure Light
Scientists use special tools and filters to measure star brightness. These filters help them measure light in specific colors or wavelengths. The table below uses a filter that measures light similar to what the human eye sees. But stars also give off light in other ways, like infrared (heat) light. A star might look dim in visible light but be very bright in infrared. For example, Betelgeuse is much brighter in infrared light than in visible light.
Stars That Change Brightness
Some stars are called variable stars because their brightness changes over time. This can happen over days, months, or even years.
- For these stars, the table shows their brightest magnitude or an average brightness.
- Betelgeuse and Antares are examples of variable stars. Their brightness can go up and down.
- For some variable stars, especially red ones, it's hard to say exactly what their "maximum" brightness is because it changes each time.
Using Standard Stars
To make sure measurements are consistent, astronomers use certain stars as "standard stars." These stars have very carefully measured brightnesses that don't change much. They help astronomers compare and measure the brightness of other stars accurately.
Star Names and Labels
All the stars on this list have several official names or numbers. The table mainly uses their Bayer designation (like "Alpha Centauri") and their most common proper name (like "Sirius"). Most of these common names have been officially approved by the International Astronomical Union (IAU), which is a group of astronomers.
Brightest Stars Table
The information in this table comes from Wikipedia articles about each star. You can find more details and references in those individual articles.
Wolf–Rayet star |
O-type star |
B-type star |
A-type star |
F-type star |
G-type star |
K-type star |
M-type star |
Brightest star of its constellation |
Rank | Visual magnitude (mV) | Proper name | Bayer designation |
Distance (ly) | Spectral type | Celestial Hemisphere |
---|---|---|---|---|---|---|
0 | −26.74 | Sun | 0.0 | G2 V | ||
1 | −1.46 | Sirius | α CMa | 8.6 | A0mA1 Va, DA2 | Southern |
2 | −0.74 | Canopus | α Car | 310 | A9 II | Southern |
3 | −0.27 (0.01 + 1.33) | Rigil Kentaurus & Toliman |
α Cen | 4.34 | G2 V, K1 V | Southern |
4 | −0.05 | Arcturus | α Boo | 37 | K0 III | Northern |
5 | 0.03 (−0.02–0.07var) | Vega | α Lyr | 25 | A0 Va | Northern |
6 | 0.08 (0.03–0.16var) | Capella | α Aur | 43 | K0 III, G1 III | Northern |
7 | 0.13 (0.05–0.18var) | Rigel | β Ori | 860 | B8 Ia | Southern |
8 | 0.34 | Procyon | α CMi | 11 | F5 IV-V | Northern |
9 | 0.46 (0.40–0.46var) | Achernar | α Eri | 139 | B3 Vpe | Southern |
10 | 0.50 (0.0–1.6var) | Betelgeuse | α Ori | 640 | M1-M2 Ia-ab | Northern |
11 | 0.61 | Hadar | β Cen | 390 | B1 III | Southern |
12 | 0.76 | Altair | α Aql | 17 | A7 V | Northern |
13 | 0.76 (1.33 + 1.73) | Acrux | α Cru | 320 | B0.5 IV, B1 V | Southern |
14 | 0.86 (0.75–0.95var) | Aldebaran | α Tau | 65 | K5 III | Northern |
15 | 0.96 (0.6–1.6var) | Antares | α Sco | 550 | M1.5 Iab-Ib, B2.5 V | Southern |
16 | 0.97 (0.97–1.04var) | Spica | α Vir | 250 | B1 III-IV, B2 V | Southern |
17 | 1.14 | Pollux | β Gem | 34 | K0 III | Northern |
18 | 1.16 | Fomalhaut | α PsA | 25 | A3 V | Southern |
19 | 1.25 (1.21–1.29var) | Deneb | α Cyg | 2,600 | A2 Ia | Northern |
20 | 1.25 (1.23–1.31var) | Mimosa | β Cru | 280 | B0.5 III, B2 V | Southern |
21 | 1.39 | Regulus | α Leo | 79 | B8 IVn | Northern |
22 | 1.50 | Adhara | ε CMa | 430 | B2 II | Southern |
23 | 1.58 (1.93 + 2.97) | Castor | α Gem | 51 | A1 V, Am | Northern |
24 | 1.62 | Shaula | λ Sco | 570 | B2 IV | Southern |
25 | 1.64 | Gacrux | γ Cru | 89 | M3.5 III | Southern |
26 | 1.64 | Bellatrix | γ Ori | 250 | B2 III | Northern |
27 | 1.65 | Elnath | β Tau/γ Aur | 130 | B7 III | Northern |
28 | 1.69 | Miaplacidus | β Car | 110 | A1 III | Southern |
29 | 1.69 (1.64–1.74var) | Alnilam | ε Ori | 2,000 | B0 Ia | Southern |
30 | 1.72 (1.81–1.87var + 4.27) | Regor | γ Vel | 840 | WC8, O7.5III | Southern |
31 | 1.74 | Alnair | α Gru | 100 | B6 V | Southern |
32 | 1.77 | Alnitak | ζ Ori | 1,300 | O9.5 Iab, B1 IV, B0 III | Southern |
33 | 1.77 | Alioth | ε UMa | 83 | A1 III-IVp kB9 | Northern |
34 | 1.79 | Dubhe | α UMa | 120 | K0 III, F0 V | Northern |
35 | 1.80 | Mirfak | α Per | 510 | F5 Ib | Northern |
36 | 1.82 | Wezen | δ CMa | 1,800 | F8 Ia | Southern |
37 | 1.84 | Sargas | θ Sco | 330 | F0 II | Southern |
38 | 1.85 | Kaus Australis | ε Sgr | 140 | B9.5 III | Southern |
39 | 1.86 | Avior | ε Car | 600 | K3 III, B2 Vp | Southern |
40 | 1.86 | Alkaid | η UMa | 100 | B3 V | Northern |
41 | 1.90 (1.89–1.94var) | Menkalinan | β Aur | 80 | A1mIV+A1mIV | Northern |
42 | 1.91 | Atria | α TrA | 390 | K2 IIb-IIIa | Southern |
43 | 1.92 | Alhena | γ Gem | 100 | A1.5 IV+ | Northern |
44 | 1.94 | Peacock | α Pav | 180 | B3 V | Southern |
45 | 1.96 (1.99–2.39var + 5.57) | Alsephina | δ Vel | 80 | A1 Va(n), F7.5 V | Southern |
46 | 1.98 | Mirzam | β CMa | 500 | B1 II-III | Southern |
47 | 2.00 | Alphard | α Hya | 180 | K3 II-III | Southern |
48 | 1.98 (1.86–2.13var) | Polaris | α UMi | 430 | F7 Ib | Northern |
49 | 2.00 | Hamal | α Ari | 66 | K1 IIIb | Northern |
50 | 2.08 (2.37 + 3.64) | Algieba | γ Leo | 130 | K0 III, G7 IIIb | Northern |
51 | 2.02 | Diphda | β Cet | 96 | K0 III | Southern |
52 | 2.04 | Mizar | ζ UMa | 83 | A2 Vp, A2 Vp, Am | Northern |
53 | 2.05 | Nunki | σ Sgr | 230 | B2.5 V | Southern |
54 | 2.06 | Menkent | θ Cen | 59 | K0 III | Southern |
55 | 2.06 | Alpheratz | α And/δ Peg | 97 | B8 IVpMnHg, A3 V | Northern |
56 | 2.07 (2.01–2.10var) | Mirach | β And | 200 | M0 III | Northern |
57 | 2.07 | Rasalhague | α Oph | 47 | A5IVnn | Northern |
58 | 2.08 | Kochab | β UMi | 130 | K4 III | Northern |
59 | 2.09 | Saiph | κ Ori | 720 | B0.5 Ia | Southern |
60 | 2.11 | Denebola | β Leo | 36 | A3 Va | Northern |
61 | 2.12 (2.1–3.39var) | Algol | β Per | 93 | B8 V, K0 IV, A7m | Northern |
62 | 2.15 (2.0–2.3var) | Tiaki | β Gru | 170 | M5 III | Southern |
63 | 2.17 | Muhlifain | γ Cen | 130 | A0 III, A0 III | Southern |
64 | 2.21 | Aspidiske | ι Car | 690 | A9 Ib | Southern |
65 | 2.21 (2.14–2.30var) | Suhail | λ Vel | 570 | K4 Ib | Southern |
66 | 2.23 (2.21–2.32var) | Alphecca | α CrB | 75 | A0 V, G5 V | Northern |
67 | 2.23 (2.23–2.35var) | Mintaka | δ Ori | 900 | O9.5 II, B1 V, B0 IV | Southern |
68 | 2.23 | Sadr | γ Cyg | 1,500 | F8 Iab | Northern |
69 | 2.23 | Eltanin | γ Dra | 150 | K5 III | Northern |
70 | 2.24 | Schedar | α Cas | 230 | K0 IIIa | Northern |
71 | 2.25 | Naos | ζ Pup | 1,080 | O4 If(n)p | Southern |
72 | 2.26 | Almach | γ And | 350 | K3 IIb, B9.5 V, B9.5 V, A0 V | Northern |
73 | 2.28 (2.25–2.31var) | Caph | β Cas | 54 | F2 III | Northern |
74 | 2.29 | Izar | ε Boo | 202 | K0 II-III, A2 V | Northern |
75 | 2.30 (2.29–2.34var) | — | α Lup | 550 | B1.5 III | Southern |
76 | 2.30 (2.29–2.31var) | — | ε Cen | 380 | B1III | Southern |
77 | 2.31 (1.6–2.32var) | Dschubba | δ Sco | 400 | B0.3 IV, B1-3 V | Southern |
78 | 2.31 | Larawag | ε Sco | 65 | K1 III | Southern |
79 | 2.35 (2.30–2.41var) | — | η Cen | 310 | B1.5 Vne | Southern |
80 | 2.37 | Merak | β UMa | 79 | A1 IVps | Northern |
81 | 2.38 | Ankaa | α Phe | 77 | K0.5 IIIb | Southern |
82 | 2.39 | Girtab | κ Sco | 460 | B1.5 III | Southern |
83 | 2.40 (0.7–3.0var) | Enif | ε Peg | 670 | K2 Ib | Northern |
84 | 2.42 (2.31–2.74var) | Scheat | β Peg | 200 | M2.5 II-IIIe | Northern |
85 | 2.43 | Sabik | η Oph | 88 | A1 IV, A1 IV | Southern |
86 | 2.44 | Phecda | γ UMa | 84 | A0 Ve | Northern |
87 | 2.45 | Aludra | η CMa | 2,000 | B5 Ia | Southern |
88 | 2.46 | Markeb | κ Vel | 540 | B2 IV | Southern |
89 | 2.47 (1.6–3.0var) | Tsih / Navi | γ Cas | 610 | B0.5 IVe | Northern |
90 | 2.48 | Markab | α Peg | 140 | A0 IV | Northern |
91 | 2.48 | Aljanah | ε Cyg | 72 | K0 III-IV | Northern |
92 | 2.50 | Acrab | β Sco | 404 | B0.5 IV-V, B1.5 V, B2 V | Southern |
Brightest Stars in Other Galaxies
Our own Milky Way galaxy has the Sun as its brightest star (from our view). But other galaxies also have their own brightest stars! Here are a few:
Galaxy | Apparent Magnitude | Star | Distance (ly) | Spectral type | Notes |
---|---|---|---|---|---|
Milky Way | –26.74 | Sun | 0 | G2V | |
Large Magellanic Cloud | 8.99 – 9.22 (variable) | HD 33579 | 163,000 | A3Ia+ | The Luminous Blue Variables S Doradus and R71 can be even brighter when they have outbursts. |
Small Magellanic Cloud | 10.47 | SK 69 | 200,000 | B8Ia | |
Andromeda Galaxy | 15.6 | [DMM2009] J004406.32+420131 | 2,500,000 | F2Ia | |
Triangulum Galaxy | 14.859 | B324 | 3,200,000 | A8–F0Ia | A yellow hypergiant, which is a very large and bright star. |
More About Stars
In Spanish: Anexo:Estrellas más brillantes para niños
- Historical brightest stars: Learn about the brightest stars in Earth's sky over millions of years.
- List of variable stars: Stars that change their brightness.
- List of most luminous stars: Stars that are truly the brightest, no matter their distance.
- List of nearest stars and brown dwarfs: Stars and star-like objects closest to us.
- Lists of stars: Find more lists about stars.