Target guide · open cluster

NGC 869 Double Cluster with a smart telescope

NGC 869 Double Cluster is a open cluster about 41 arcminutes (0.68°) across, magnitude 3.7. It is highest around midnight in October, best placed for the northern hemisphere, and bright enough to image from a suburb or even a city. Of the 14 smart telescopes we track, Seestar S30, DWARF mini, Seestar S50 Pro frame it best.

Key facts

CatalogueNGC 869
Typeopen cluster
Apparent size41′ × 15′
Magnitude3.7
Position (J2000)RA 2.35 h, Dec 57.1°
Highest at midnightOctober (±2 weeks)
Sky neededCity-friendly surface brightness 19.3 mag/arcsec²

In the best-matching frame

NGC 869 · 41′ × 15′
NGC 869 Double Cluster (blue) inside the native frame of Seestar S30 (2.14° × 1.21°).

Simulate your photo of Double Cluster →

Imaging tips

Star clusters and star groups are bright and forgiving: they show well from a city and need only short sessions. A wider field of view shows the whole group with some surrounding sky. Double Cluster is one of the easier targets from light-polluted skies.

Which smart telescope frames it best

TelescopeField of viewFitMosaic
ZWO Seestar S302.14° × 1.21°fits wellone frame
DWARFLAB DWARF mini2.13° × 1.2°fits wellone frame
ZWO Seestar S50 Pro2.45° × 1.38°fits wellone frame
Vaonis Vespera II2.5° × 1.4°fits wellone frame
Vaonis Vespera 32.5° × 1.4°fits wellone frame
Vaonis Vespera Pro 21.6° × 1.6°fits wellone frame
DWARFLAB DWARF 32.93° × 1.65°fits wellone frame
ZWO Seestar S30 Pro3.99° × 2.24°fits wellone frame
Celestron Origin Mark II1.32° × 0.75°fits wellone frame
ZWO Seestar S501.29° × 0.73°fits wellone frame
Unistellar eQuinox 20.76° × 0.57°larger than the frame2 × 1 = 2 panels
Unistellar eVscope 20.76° × 0.57°larger than the frame2 × 1 = 2 panels
Unistellar Odyssey0.75° × 0.56°larger than the frame2 × 1 = 2 panels
Unistellar Odyssey Pro0.75° × 0.56°larger than the frame2 × 1 = 2 panels

Mosaic planner

Double Cluster is larger than the frame of some smart telescopes. A mosaic covers it with several overlapping frames that are stitched together afterwards. Pick a telescope to see the layout.

12
Odyssey · 0.75° × 0.56°: 2 × 1 = 2 panels Each panel needs its own exposure, so plan about 2× the imaging time of a single frame.

Calculated with 15% overlap between panels and a 10% margin around the object, with the frame lined up along the object's long axis. When the object is longer than the short side of the frame we always count at least two panels, because on an alt-az mount the frame turns during the night. Whether a telescope has a built-in mosaic mode depends on its app and firmware; you can also shoot the panels separately and stitch them yourself.

How high it gets from where you live

Highest altitude above a flat horizon. Below about 20° the image suffers from haze and light pollution; trees and roofs often block it completely.

LatitudeHighest altitude
Oslo, 60° N87°
Amsterdam, 52° N85°
Madrid, 40° N73°
Miami, 26° N59°
Equator33°
Sydney, 34° Snever rises
See if it clears your own horizon tonight

Nearby in the sky

Objects close to NGC 869 in the sky, so you can image them in the same session.

Questions and answers

Can I photograph NGC 869 Double Cluster from a city?
Yes. It is bright enough to image from a suburb or even a city.
Which smart telescope is best for NGC 869 Double Cluster?
Seestar S30, DWARF mini, Seestar S50 Pro frame it best in a single frame, based on its size and each telescope's field of view.
When is the best time to photograph NGC 869 Double Cluster?
It is highest around midnight in October and best placed for the northern hemisphere. From 52° north it climbs to about 85° at most.

Object data: Messier catalogue via d3-celestial (BSD-3); NGC and IC objects from OpenNGC (CC BY-SA 4.0). Altitudes and dates are calculated, not observed.