No products in the cart.

Hubble Examines Low Brightness, High Interest Galaxy

Explore Hubble

Hubble Home
Overview

About Hubble
The History of Hubble
Hubble Timeline
Why Have a Telescope in Space?
Hubble by the Numbers
At the Museum
FAQs

Impact & Benefits

Hubble’s Impact & Benefits
Science Impacts
Cultural Impact
Technology Benefits
Impact on Human Spaceflight
Astro Community Impacts

Science

Hubble Science
Science Themes
Science Highlights
Science Behind Discoveries
Hubble’s Partners in Science
Universe Uncovered
AI and Hubble Science
Explore the Night Sky

Observatory

Hubble Observatory
Hubble Design
Mission Operations
Missions to Hubble
Hubble vs Webb

Team

Hubble Team
Career Aspirations
Hubble Astronauts

Multimedia

Images
Videos
Sonifications
Podcasts
e-Books
Online Activities
3D Hubble Models
Lithographs
Fact Sheets
Posters
Hubble on the NASA App
Glossary

News

Hubble News
Social Media
Media Resources

More

35th Anniversary
Online Activities

2 min read
Hubble Examines Low Brightness, High Interest Galaxy

This NASA/ESA Hubble Space Telescope image features a portion of the spiral galaxy NGC 45.
ESA/Hubble & NASA, D. Calzetti, R. Chandar; Acknowledgment: M. H. Özsaraç

This NASA/ESA Hubble Space Telescope image zooms in on the feathery spiral arms of the galaxy NGC 45, which lies just 22 million light-years away in the constellation Cetus (the Whale).
The portrait uses data drawn from two complementary observing programs. The first took a broad view of 50 nearby galaxies, leveraging Hubble’s ability to observe ultraviolet through visible into near-infrared light to study star formation in these galaxies. The second program examined many of the same nearby galaxies as the first, narrowing in on a particular wavelength of red light called H-alpha. Star-forming nebulae are powerful producers of H-alpha light, and several of these regions are visible across NGC 45 as bright pink-red patches.
These observing programs aimed to study star formation in galaxies of different sizes, structures, and degrees of isolation — and NGC 45 is a particularly interesting target. Though it may appear to be a regular spiral galaxy, NGC 45 is a remarkable type called a low surface brightness galaxy.
Low surface brightness galaxies are fainter than the night sky itself, making them incredibly difficult to detect. They appear unexpectedly faint because they have relatively few stars for the volume of gas and dark matter they carry. In the decades since astronomers serendipitously discovered the first low surface brightness galaxy in 1986, researchers have learned that 30–60% of all galaxies may fall into this category. Studying these hard-to-detect galaxies is key to understanding how galaxies form and evolve, and Hubble’s sensitive instruments are equal to the task.
Text Credit: ESA/Hubble

Facebook logo

@NASAHubble

@NASAHubble

Instagram logo

@NASAHubble

Share

Details

Last Updated

Aug 14, 2025

Editor

Andrea Gianopoulos

Location

NASA Goddard Space Flight Center

Related Terms

Astrophysics
Astrophysics Division
Galaxies
Galaxies, Stars, & Black Holes
Hubble Space Telescope
Spiral Galaxies
Star-forming Nebulae
Stars
The Universe

Keep Exploring
Discover More Topics From Hubble

35 Years of Hubble Images

Hubble’s Night Sky Challenge

Hearing Hubble

3D Hubble Models