---
title: "NGC 7769"
url: "https://spacecatalog.org/object/ngc-7769"
release: "DR1"
licence: "CC-BY-SA-4.0"
citation: "SpaceCatalog. NGC 7769 [catalogue entry]. Data release DR1 (2026-08-21). https://spacecatalog.org/object/ngc-7769"
---

# NGC 7769

NGC 7769 is a spiral [galaxy](https://spacecatalog.org/galaxies) Sb in the constellation [Pegasus](https://spacecatalog.org/constellation/pegasus), 179.1 Mly from Earth, shining at apparent magnitude 11.79 (V). Other catalogues list it as 2MASX J23510396+2009014, IRAS 23485+1952 and IRAS F23485+1952, among 9 designations in total. It was discovered in 1784.

## At a glance

- **WHAT IT IS:** Spiral galaxy
- **HOW FAR:** 179.1 Mly — A luminosity distance, from its redshift — how faint it looks. The light itself left 192 million years ago.
- **HOW BIG ON THE SKY:** 1.8′ — Small enough that the full Moon would cover it several times over.
- **HOW BRIGHT (V):** 11.79 — A small telescope reaches it.
- **WHERE TO LOOK:** [Pegasus](https://spacecatalog.org/constellation/pegasus) — The patch of sky it sits in, as seen from Earth.

## Properties

| Quantity | Value |
| --- | --- |
| CLASS | Spiral galaxy Sb |
| DISTANCE FROM EARTH | 179.1 Mly ±16 — by redshift (CMB frame), flat ΛCDM with H0 = 70 km/s/Mpc |
| APPARENT MAGNITUDE (V) | 11.79 |
| CONSTELLATION | Pegasus |
| RIGHT ASCENSION (J2000) | 23h 51m 04.0s |
| DECLINATION (J2000) | +20° 09′ 01.5″ |
| DISCOVERED | 1784 |

## Catalogue data

### WHAT KIND OF THING IT IS

What the object is in itself, rather than how it happens to look from here.

| Field | Value |
| --- | --- |
| Hubble type | Sb |

### HOW BRIGHT IT IS

What the light adds up to, measured through one filter at a time. A magnitude is a brightness on a backwards scale — the smaller the number, the brighter the object.

| Field | Value |
| --- | --- |
| Apparent magnitude (B) | 12.50 |
| Apparent magnitude (V) | 11.79 |
| Apparent magnitude (J) | 9.90 |
| Apparent magnitude (H band) | 9.21 |
| Apparent magnitude (K) | 8.93 |
| Surface brightness | 21.79 mag/arcsec² |

### WHERE IT IS AND HOW IT MOVES

Position, motion across the sky and the size it covers on it. These are measurements of the object as seen from here, so every one of them depends on where here is.

| Field | Value |
| --- | --- |
| Radial velocity | 4138 km/s |
| Redshift (z) | 0.0139 |
| Redshift (z, CMB frame) | 0.0126994 |
| Major axis | 1.75′ |
| Minor axis | 0.67′ |
| Position angle | 85° |

### WHEN IT WAS FOUND

Who first saw it, from where, and by what method.

| Field | Value |
| --- | --- |
| Discovered by | William Herschel |

### OTHER NAMES AND NUMBERS

The identifiers other catalogues file this object under, for anyone joining this data to theirs.

| Field | Value |
| --- | --- |
| OpenNGC type code | G |
| Wikidata item | Q784327 |
| Wikipedia article | NGC 7769 |

## Also known as

- 2MASX: 2MASX J23510396+2009014
- IRAS: IRAS 23485+1952
- IRAS: IRAS F23485+1952
- LEDA: LEDA 72615
- MCG: MCG +03-60-030
- NGC: NGC 7769
- NGC: NGC 7771W
- PGC: PGC 72615
- UGC: UGC 12808

## Source

[OpenNGC](https://github.com/mattiaverga/OpenNGC) — CC-BY-SA-4.0

The producer asks: OpenNGC, Mattia Verga (github.com/mattiaverga/OpenNGC). Fields derived from it stay under CC BY-SA 4.0.

How this was made: https://spacecatalog.org/methods#source-openngc

## Cite this page

SpaceCatalog. NGC 7769 \[catalogue entry\]. Data release DR1 (2026-08-21). https://spacecatalog.org/object/ngc-7769

```bibtex
@misc{spacecatalog_ngc-7769,
  author       = {{SpaceCatalog}},
  title        = {{NGC 7769}},
  howpublished = {SpaceCatalog, data release DR1 (2026-08-21)},
  year         = {2026},
  url          = {https://spacecatalog.org/object/ngc-7769},
  note         = {Catalogue entry, data release DR1 (2026-08-21). Values from OpenNGC.}
}
```

OpenNGC — CC-BY-SA-4.0

Acknowledgement the producer asks for: OpenNGC, Mattia Verga (github.com/mattiaverga/OpenNGC). Fields derived from it stay under CC BY-SA 4.0.

The page itself, with its pictures, the sky map and the observing tools: https://spacecatalog.org/object/ngc-7769
