The Spiral Cluster

M34 / NGC 1039 • Perseus

The Spiral Cluster
1. The blue-white main sequence stars
The Spiral Cluster
2. M34 in the Perseus star field

A Sparking Jewel Box

M34 is a group of about 100 stars that formed together approximately 200 million years ago. It is roughly the same age as the famous Pleiades, but it is located further away. The cluster is dominated by bright blue-white stars, but keen-eyed observers (and sensitive cameras) will notice several yellow and orange giants scattered throughout, which have already begun to evolve off the main sequence. It is a perfect example of a 'young' cluster that is just beginning to disperse into the Milky Way.

Imaging Challenges

  • • Star Color: Open clusters are all about the 'hue.' Using SPCC is vital to ensure the blue stars look blue and the orange stars look orange, rather than everything just being white.
  • • Dynamic Range: To keep the stars from 'bloating' or losing their color in the centers, you must use shorter exposures or careful HDR processing.
  • • Background Uniformity: Because there is no nebula to hide behind, any gradients or sensor noise will be very apparent in the empty space between the stars.
M34 spans an area of the sky nearly as large as the full moon.

Astro Data

Distance 1,500 Light Years
Object Type Open Cluster
Constellation Perseus

Acquisition

Telescope Sharpstar 130HNT
Camera Player One Uranus-C Pro
Integration 2-4 hours Hours
Integration UV/IR Cut (Broadband) Hours
m13.html Cluster
m44.html Cluster

Bring the Cosmos Home

The The Spiral Cluster offers a unique and complex aesthetic for any modern collection.

All images are available as limited edition, museum-quality fine art prints...

Inquire About Prints