Auriga Constellation: How to Find Capella, Its Stars and Star Clusters

By · Published on · Details checked on 30 September 2026

Auriga, the Charioteer, is a winter constellation and home to Capella, the sixth-brightest star in the night sky. It covers 657 square degrees, sits above Orion and in January passes almost straight overhead across much of the United States.

More in our overview: Constellations.

⭐ The short version: To find Auriga, go about 40 degrees straight up from Betelgeuse in Orion – that is where the yellowish Capella shines. The best time is on evenings from December to February. What makes it special: in mid-January Capella stands 85 degrees high in New York around 9:30 p.m., nearly at the zenith, and north of 44° N – Seattle, Minneapolis – it never sets at all.
Finder chart: from Betelgeuse in Orion 40 degrees up to Capella in the Auriga constellation, with M 36, M 37 and M 38
From Betelgeuse straight up to Capella. Graphic: sterngucker.de, own calculation

At a glance

Latin nameAuriga (the Charioteer)
Area657 square degrees (rank 21 of 88)
Brightest starCapella, magnitude 0.08, just under 43 light-years
Best time to observeevenings from December to February
Peak altitude of Capella88° in Seattle, 85° in New York, 77° in Dallas
CircumpolarCapella yes, north of 44° N (e.g. Seattle, Minneapolis); farther south it sets for a few hours
NeighborsCamelopardalis, Perseus, Taurus, Gemini, Lynx
Best-known deep-sky objectsopen star clusters M 36, M 37 and M 38
Altitudes calculated as 90° − |latitude − declination| (Capella: +46.0°).

How to find the Auriga constellation

On a winter evening, Orion is your signpost. From reddish Betelgeuse, his left shoulder, go about 40 degrees straight up – roughly four hand widths at arm’s length. The brightest star you run into there is Capella.

Halfway there you pass Elnath, 22 degrees above Betelgeuse. Elnath forms the bottom point of the pentagon that it makes together with Capella, Menkalinan, Mahasim and Hassaleh. The figure stands above Orion like a lopsided house with a pointed roof.

Double check: 3 to 5 degrees below and to the right of Capella sits a small, narrow triangle of stars – the “Kids”, ε, ζ and η Aurigae. If you can see it, you have definitely found Capella.

In the fall, the Orion method does not work yet. Then Capella rises low in the northeast in the evening and often twinkles in surprisingly vivid colors – an effect of the thick layer of air near the horizon. Our guide to the stars helps you tell which bright star is which.

The stars of Auriga

StarMagnitudeDistanceType
Capella (α Aur)0.08just under 43 light-yearstwo yellow giants G8 III + G0 III
Menkalinan (β Aur)1.90about 81 light-yearseclipsing binary, A-type
Mahasim (θ Aur)2.62about 166 light-yearswhite star A0p, double star
Hassaleh (ι Aur)2.69about 450 light-yearsorange giant K3 II
Almaaz (ε Aur)2.99uncertain, 2,000–3,500 light-yearssupergiant F0, eclipsing binary
Haedus (η Aur)3.18about 233 light-yearsblue main-sequence star B3 V
Saclateni (ζ Aur)3.75about 860 light-yearsK5 II + B7 V, eclipsing binary
Elnath (magnitude 1.65) is left out on purpose: since the IAU drew the official boundaries, it belongs to Taurus.

A striking number of these stars are eclipsing binaries. Menkalinan, Almaaz and Saclateni are double stars whose partners block each other as seen from Earth – for Menkalinan every 3.96 days, although you will hardly notice it.

Elnath used to be the star γ Aurigae. Today it officially belongs to the Taurus constellation, where it marks the tip of the northern horn. It is still drawn as part of the Charioteer’s figure.

Capella: the star in Auriga

Capella means “little she-goat”. At magnitude 0.08 it is the sixth-brightest star in the entire sky and, after Arcturus and Vega, the third-brightest in the northern sky. Its yellowish hue resembles our Sun.

In fact, Capella is not a single star. It is two yellow giant stars of about two and a half solar masses each, orbiting each other in just 104 days. They are roughly 12 and 9 times the Sun’s diameter, and each shines about 75 times as bright as the Sun.

You cannot split the two. They are only 0.74 astronomical units apart – less than the Sun–Earth distance – which from just under 43 light-years can only be measured with interferometers (large telescopes linked together). A pair of faint red dwarfs orbits much farther out.

Common misconception: Many people take the colorfully flashing Capella low in the northeast on fall evenings for a planet, an aircraft or something unexplained. The color show happens in our atmosphere. Once Capella climbs higher later in the night, it shines calmly and yellowish.

Why Capella passes almost overhead

Capella has a declination of +46.0 degrees. At exactly 46 degrees north – just north of Portland, Oregon, and Minneapolis – it passes straight overhead. It reaches 89 degrees in Minneapolis, 88 in Seattle, 85 in New York and still 70 degrees in Miami.

Chart: highest and lowest altitude of Capella in eleven US cities and its altitude at 10 p.m. in New York over the year
Left: highest and lowest point per city; right: altitude at 10 p.m. over the year. Graphic: sterngucker.de, own calculation

The second consequence of this high declination: Capella is circumpolar and never sets north of 44 degrees latitude. At its lowest point in the north it still stands 4 degrees high in Seattle and 1 degree in Minneapolis. From Boston southward it dips below the northern horizon for a while – about 2.5 hours in Boston, 3.6 in New York and 8 hours in Miami.

For observing, this means: in winter Auriga sits right above you in the best seeing, far from the haze near the horizon. Looking straight up is uncomfortable, though – a reclining lawn chair helps.

When Auriga is visible

Auriga is a classic winter constellation. From late November to mid-February, Capella stands higher than 60 degrees at 10 p.m., highest in mid-January.

MonthAltitude at 10 p.m.DirectionCulmination
September8°northeast6:34 a.m.
October23°northeast4:36 a.m.
November51°northeast1:34 a.m.
December72°northeast11:36 p.m.
January83°almost overhead, slightly north9:32 p.m.
February63°northwest7:30 p.m.
March54°northwest6:40 p.m.
April to June34° to 4°northwestafternoon
July and Augustbelow the horizon (−3° to −1°)northmorning
Calculated for New York, on the 15th of each month (EST or EDT). Other US cities differ by up to about half an hour and a few degrees.

In summer, little is left of Auriga. In mid-June the Sun passes only a good 5 degrees from Elnath, and the southern part of the figure sets in daylight. Capella itself hugs the northern horizon in the short nights or, in most of the US, dips below it.

The Sun never enters Auriga on its yearly path. That is why it is not a zodiac constellation, unlike its neighbor Taurus. And if you ever want to observe the Sun during the day: only with a certified front-mounted solar filter.

M 36, M 37 and M 38: three star clusters in a row

In the middle of the pentagon lie three open star clusters – loose groups of young stars born together. M 38, M 36 and M 37 line up almost perfectly, just under 6 degrees long in total. They are between about 3,700 and 4,900 light-years away.

ClusterMagnitudeSizeDistance
M 366.012 arcminutesabout 3,900 light-years
M 375.623 arcminutesabout 4,900 light-years
M 386.420 arcminutesabout 3,700 light-years
Distances from Gaia parallaxes (SIMBAD). For comparison: the full Moon measures about 30 arcminutes.

In binoculars they look like three small fuzzy patches. Only a telescope resolves them into individual stars – M 37 is the richest and most beautiful, with a dense core of hundreds of faint stars. M 36 looks loose and bright by comparison, while M 38 shows a striking cross shape.

How to find them: Start at Elnath and sweep about 6 degrees up, slightly toward Mahasim – that is where M 36 lies. M 38 follows 2.3 degrees farther up and to the right, and M 37 lies 3.7 degrees down and to the left – just as on the finder chart above.

Epsilon Aurigae: the star with the 27-year eclipse

Almaaz, only 3.4 degrees from Capella, is one of the most puzzling stars of all. Every 27.1 years a huge, dark disk of dust slides in front of the supergiant and dims it for almost two years from magnitude 2.9 to 3.8.

The last eclipse ran from 2009 to 2011. By our calculation, the next one begins in the fall of 2036, with mid-eclipse in 2037. You will be able to see the drop in brightness with the naked eye by comparing Almaaz with the neighboring Kids.

Mythology: charioteer and goat

The figure combines two legends. The Charioteer himself is usually identified as Erichthonius, revered as the inventor of the four-horse chariot; other traditions see him as the charioteer Myrtilus.

On his shoulder he carries a goat. Capella is the goat Amalthea, who nursed the infant Zeus with her milk, and the Kids next to her are her young. That is also where the names Capella (“little she-goat”) and Haedus (“young goat”) come from.

Binoculars or telescope

For Auriga, the telescope wins. M 36, M 37 and M 38 are small enough that only aperture and magnification reveal their stars – aperture means the diameter of the main optics, which determines how much light it collects. A pair of Celestron 7x50 Cometron BinocularsCelestron UpClose G2 10x50 Porro Binoculars is enough to find the three patches, but not much more.

Tip for beginners: A small tabletop Dobsonian with 130 mm (5.1 in) of aperture already shows M 37 as a sparkling star field. Use the eyepiece with the lowest magnification – then the loose clusters fit completely into the view.

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When more aperture pays off

More aperture mainly shows you more faint stars. M 37 in particular gains with every millimeter, because its dense core consists of very faint members.

If you want more: the next step
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Frequently asked questions about the Auriga constellation

How do I find the Auriga constellation?

In winter, go about 40 degrees straight up from Betelgeuse in Orion – roughly four hand widths. There you will find the bright, yellowish Capella. Auriga’s pentagon closes below it with Elnath.

What does Auriga mean?

Auriga is the Latin name of the constellation and means charioteer. In crosswords, AURIGA (6 letters) is the usual answer for “the Charioteer constellation”. The IAU abbreviation is Aur.

How bright is the star Capella and how far away is it?

Capella shines at magnitude 0.08, making it the sixth-brightest star in the night sky. It is just under 43 light-years away. Behind the point of light are two yellow giant stars that orbit each other in 104 days.

Is Auriga visible all year?

North of 44 degrees – Seattle, Minneapolis – Capella never sets; farther south it dips below the northern horizon for a few hours each day. In summer it stands at most a few degrees above the northern horizon and gets lost in the twilight. You can see the whole figure well from November to March.

Which star clusters are in Auriga?

The best known are the open star clusters M 36, M 37 and M 38, all between magnitude 5.6 and 6.4. In binoculars they are small patches; in a telescope they resolve into stars. M 37 is considered the most beautiful of the three.

Does Elnath belong to Auriga or to Taurus?

Officially to Taurus, where it is called β Tauri. It used to be listed as γ Aurigae as well. Star charts still usually draw it as a corner of Auriga’s pentagon.

When is the next eclipse of Epsilon Aurigae?

The period is 27.1 years, and the last eclipse ran from 2009 to 2011. By our calculation, the next one begins in the fall of 2036 and lasts almost two years. You can follow it with the naked eye.

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