The Orion Nebula


Orion NebulaThe Orion Nebula (also known as Messier 42, M42, or NGC 1976) is one of the brightest nebulae, and is visible to the naked eye even in areas affected by minor light pollution. It is seen as the middle “star” in the sword of Orion, the three stars located below Orion’s Belt. The “star” appears fuzzy to sharp-eyed observers, and its nebulosity is obvious through binoculars or a small telescope.

Image Credit: NASA

Galactic Onion


Galactic onionThis is NGC 3923, an example of a shell galaxy in which the stars in its halo are arranged in layers. Roughy ten percent of all elliptical galaxy exhibits this onion-like structure. The shell-like structures are thought to result from galactic cannibalism when a larger galaxy swallows a smaller companion. As the galactic centers approach, they initially oscillate about a common center. Ripples flow outwards forming the shells of stars, a three dimensional equivalent of ripples on a pond spreading across its surface. NGC 3923 has over twenty shells, but only a few of the outer ones visible in this picture.

Image Credit: ESA / NASA

The Eagle in 3D


3D data visualisation of the Pillars of CreationEagle_nebula_pillars smallMany of the Gentle Readers will remember the iconic image on the left of the Pillars of Creation in the Eagle Nebula (aka Messier 16) made famous in a picture from the Hubble Space Telescope. Using the Multi Unit Spectroscopic Explorer instrument on European Southern Observatory’s  Very Large Telescope, astronomers have produced the first complete three-dimensional view.

The VLT observations show how the different dusty pillars are distributed in space and reveal many new details, including a previously unknown jet from a young star. Intense radiation and stellar winds from the cluster’s brilliant stars have shaped the Pillars of Creation over time and will blow them away over the next three million years.

Image Credit: ESO

The Oyster Nebula


A hazy nebulaThis is a false color image from Hubble’s Wide Field Planetary Camera 2 of NGC 1501, a complex planetary nebula located in the constellation of Camelopardalis (The Giraffe). NGC 1501 is a planetary nebula that is just under 5,000 light-years away from us. It has a central star shining brightly from within the nebula’s cloud. This bright pearl embedded in its glowing shell gives rise to the nebula’s popular nickname—the Oyster Nebula.

While NGC 1501’s central star blasted off its outer shell long ago, it still remains very hot and luminous, but it can be difficult to spot through modest telescopes. The star seems to be pulsating, varying quite significantly in brightness over a timescale of just half an hour. While variable stars are not unusual, it is unusual to find one at the heart of a planetary nebula.

Image Credit: ESA / NASA

I Zwicky 18


I_Zwicky_18I Zwicky 18 is a dwarf irregular galaxy located about 59 million light years away. Spectroscopic observations with ground-based telescopes showed that I Zwicky 18 to be almost completely made up of hydrogen and helium, the main ingredients created in the Big Bang, and galaxies with I Zwicky 18’s youthful appearance are typically found only in the early universe. Initial observations with the Hubble Space Telescope suggested an age of 500 million years, but later Hubble observations found faint, older stars in the galaxy, suggesting its star formation started at least one billion years ago and possibly as much as ten billion years ago. It’s possible that the galaxy may have formed around the same time as most other galaxies.

Image Credit: NASA / ESA

Happy 25th Birthday, Hubble


This animation provides a 3D perspective on Hubble‘s 25th anniversary image of the nebula Gum 29 and the star cluster Westerlund 2 at its core. It begins fly past foreground stars and approaches the rim of the nebula. After passing through the wispy darker clouds on the near side, the simulation shows the bright gas illuminated by the intense radiation of the new stars forming in the Westerlund 2 cluster. The pillars of dark, dense gas are being sculpted by light and strong stellar winds from thousands of stars. This visualization is intended to be a scientifically reasonable interpretation, but distances within the model have been significantly compressed.

Video Credit: NASA, ESA, G. Bacon, L. Frattare, Z. Levay, and F. Summers (Viz3D Team, STScI), and J. Anderson (STScI)
Acknowledgment: The Hubble Heritage Team (STScI/AURA), A. Nota (ESA/STScI), the Westerlund 2 Science Team, and ESO