Menu

Messier 45 — Open Cluster in Taurus

Pleiades, Seven Sisters or Subaru

Open Cluster Showpiece (89/100)
Magnitude 1.6m OpenCluster Taurus Visible
Star Map
+ List + Plan Star Hop

About M45

Description

The Pleiades (also known as the Seven Sisters or Subaru) is one of the nearest and most obvious open star clusters in the sky, located about 444 light-years away in Taurus. The cluster contains over 1,000 stars, though only six to seven are easily visible to the naked eye. The brightest members are hot blue B-type stars that formed together roughly 100 million years ago. The cluster is currently passing through an unrelated dust cloud, creating the famous blue reflection nebulosity visible in photographs.

Observing Tips

Best viewed with the naked eye or binoculars rather than a telescope — the cluster spans about 2 degrees (four full Moon widths), which overfills most telescope eyepieces. The naked eye typically reveals 6-7 stars; keen-eyed observers from dark sites may count 10-14. Binoculars (7x50 or 10x50) frame the cluster perfectly and reveal dozens of fainter members cascading between the bright stars. Long-exposure photographs reveal the blue reflection nebulae around the brightest stars, but these are extremely difficult visually, requiring excellent skies and a large aperture. Best observed from October through March.

History

Known since prehistory and referenced in the writings of Homer, Hesiod, and the Bible (Book of Job). The name 'Pleiades' comes from Greek mythology — the seven daughters of Atlas and Pleione. Nearly every culture worldwide has myths about this cluster. Galileo was the first to observe the cluster telescopically in 1610, revealing many more stars than visible to the naked eye. The Japanese name 'Subaru' is now famous as the car manufacturer's logo, which depicts the cluster.

Fun Facts

The Pleiades were used by the ancient Greeks as a test of eyesight — being able to count seven or more stars indicated good vision. The cluster is slowly dispersing and will cease to exist as a cluster in about 250 million years. The reflection nebulae around the Pleiades are not the remnants of the gas from which the stars formed (that dispersed long ago) — they are an unrelated dust cloud the cluster happens to be moving through.

Observe

1Properties

Magnitude 1.6
Angular Size 110 arcmin
Distance 445 ly
Open Cluster [Distance: 445 ly]

Position & Identifiers

RA 03h 47m 24.0s
Dec +24° 07' 00.0"
Constellation Taurus
Catalog M45
Physical size
13 light-years across — about 1.6× the Sun-to-Sirius distance

2How easy to spot?

Sign in and configure your equipment and default location to see a personalized row.
Telescope Bortle 3 Bortle 4 Bortle 5
80mm refr. Easy Easy Easy
150mm Newt. Easy Easy Easy
C8 203mm Easy Easy Easy
Easy Medium Hard Very hard Impossible

Bortle 3 = rural · 4 = outer suburbs · 5 = suburbs

Easy on Seestar S50
At 150mm under B5 skies you should resolve about 243 of 800 members.

3Visibility

Set a location in User Settings to see visibility data.

Best season Oct – Dec (peak: Nov)

4 Eyepiece View

Log in to set your own equipment
19x TFOV: 2.3° Lim. mag: 13.6
N E

M45 · 110.0′ diameter

5 Best Magnification

6Where this cluster sits in time

1 Myr 10 Myr 100 Myr 1 Gyr 10 Gyr NGC 2362 Hyades M67 NGC 188 M45 78 Myr

Open clusters span more than four orders of magnitude in age — from newborn OB associations to ancient, metal-rich survivors.

7 Colour-Magnitude Diagram

A cluster's colour-magnitude diagram reveals its age: the bluer the turn-off point where the main sequence bends into red giants, the younger the cluster.

Loading member data…

Each point is a Gaia-DR3 member. Colour encodes spectral type; size reflects membership probability.

Discover

8

Light Travel Time Machine

9

Relativistic Travel

Community Photos (2)

Credit: NASA, ESA, AURA/Caltech, Palomar Observatory\n\nThe science team consists of: D. Soderblom and E. Nelan (STScI), F. Benedict and B. Arthur (U. Texas).... License: Public domain. (Wikimedia Commons)

Credit: NASA, ESA, AURA/Caltech, Palomar Observatory\n\nThe science team consists of: D. Soderblom and E. Nelan (STScI), F. Benedict and B. Arthur (U. Texas).... License: Public domain. (Wikimedia Commons)

Skybred Feb 28, 2026

Hamburg 2026

Hamburg 2026

Skybred Feb 28, 2026

}