Supermaxman/esa-hubble huggingface dataset:
M101 composite image: Chandra data (blue component): The blue colour shows Chandra's view in X-ray light. Sources of X-rays include million-degree gas, exploded stars, and material colliding around black holes.

Name: Messier 101, NGC 4547, Pinwheel
Type: Local Universe : Galaxy : Type : Spiral
Category: Galaxies
Constellation: Ursa Major
Distance: 22 million light years
Release date: 10 February 2009, 15:00
Credit: NASA, CXC, and K. Kuntz (JHU)

Spitzer image of M101: The galaxy Messier 101 is a swirling spiral of stars, gas, and dust. Messier 101 is nearly twice as wide as our Milky Way galaxy. Spitzer's view, taken in infrared light, reveals the galaxy's delicate dust lanes as yellow-green filaments. Such dense dust clouds are where new stars can form. In this image, dust warmed by the light of hot, young stars glows red. The rest of the galaxy's hundreds of billions of stars are less prominent and form a blue haze. Astronomers can use infrared light to examine the dust clouds where stars are born.

Name: Messier 101, NGC 4547, Pinwheel
Type: Local Universe : Galaxy : Type : Spiral
Category: Galaxies
Constellation: Ursa Major
Distance: 22 million light years
Release date: 10 February 2009, 15:00
Credit: NASA, Jet Propulsion Laboratory/Caltech and K. Gordon (STScI)

Hubble image of M101: This image shows spiral galaxy Messier 101.

Name: Messier 101, Pinwheel
Type: Local Universe : Galaxy : Type : Spiral
Category: Galaxies
Constellation: Ursa Major
Distance: 22 million light years
Release date: 10 February 2009, 15:00
Credit: NASA, ESA, CXC, SSC, and STScI

Chandra image of M101: Chandra's image of Messier 101, taken in X-ray light, shows the high-energy features of this spiral galaxy. X-rays are generally created in violent and/or high-temperature events. The white dots are X-ray sources that include the remains of exploded stars as well as material colliding at extreme speeds around black holes. The pink and blue colours are emission from million-degree gas and from clusters of massive stars. The pink emission indicates lower-energy X-rays and the blue higher-energy X-rays. One reason astronomers study Messier 101's X-rays is to better understand how black holes grow in spiral galaxies.

Name: Messier 101, NGC 4547, Pinwheel
Type: Local Universe : Galaxy : Type : Spiral
Category: Galaxies
Constellation: Ursa Major
Distance: 22 million light years
Release date: 10 February 2009, 15:00
Credit: NASA, CXC and K. Kuntz (JHU)

HST ACS/WFC image of NGC 3021: This is a NASA/ESA Hubble Space Telescope photo of the spiral galaxy NGC 3021. This was one of several hosts of recent Type Ia supernovae observed by astronomers to refine the measure of the universe's expansion rate, called the Hubble constant.

Name: NGC 3021
Type: Local Universe : Star : Type : VariableLocal Universe : Galaxy : Type : Spiral
Category: Stars
Constellation: Leo Minor
Distance: 90 million light years
Release date: 7 May 2009, 15:00
Credit: NASA, ESA and A. Riess (STScI/JHU)