NGC 613


A spiral galaxy’s brights and darksNGC 613 is a barred spiral galaxy about 65 million light-years away in the constellation of The Sculptor. It’s core looks bright and uniformly white in this image as a result of the combined light shining from the high concentration of stars packed into the core, but a massive black hole lurks at the center of this brilliance. Its mass is estimated at about 10 times that of the Milky Way’s supermassive black hole, and it is consuming stars, gas, and dust. As matter descends into the black hole’s, it radiates energy, but when looking at the galaxy in the optical and infrared wavelengths used to take this image, there is no trace of its dark heart.

Image Credit: ESA / NASA

A Bipolar Nebula


PN Hb 12A bipolar nebula, such as PN Hb 12 shown here, is not one that is off its meds. It’s a distinctive type of nebular formation characterized by an axially symmetric bi-lobed appearance.

The exact cause of this nebular structure is not known, it may be related to a physical process in which a star ejects highly energetic streams of outflow along both poles which may then collide with material surrounding the star, perhaps stellar dust or shells of matter thrown off in a prior supernova event.

Image Credit: NASA

The Medusa Merger


The Medusa Merger (aka NGC 4194) is a pair of interacting galaxies in the constellation Ursa Major. As one galaxy has consumed a smaller gas-rich system, throwing out streams of stars and dust into space, which resemble the writhing snakes that Medusa, a monster in Greek mythology famously had on her head in place of hair. Its gas-rich central region, the Eye of Medusa, is an area of extremely intense star formation.

Image Credit: NASA / ESA

Mergers and Acquisitions


NGC 2207 is a pair of colliding spiral galaxies. Although individual stars are too far apart to collide, the material between them combines to create high-density pockets of gas. Those, in turn, gravitationally collapse, triggering a firestorm of star birth. This galaxy collision will go on for several millions of years, leaving the galaxies’ shapes completely altered.

This animation combines data from three satellite observatories. Optical: Hubble data shows trails of stars and gas trace out spiral arms, stretched by the tidal pull between the galaxies. Infrared: Spitzer data reveals the glow of warm dust; raw material for the creation of new stars and planets. X-ray: Chandra view reveals areas of active star formation and the birth of super star clusters.

Video Credit: STScI

Not Quite Dead Yet


The dwarf elliptical galaxy Messier 110 may not look like much, but our near neighbor is an unusual example of its type. M110 is a member of the Local Group, the gathering of galaxies that includes the Milky Way and the galaxies closest to it. Messier 110 is one of the small satellite galaxies circling the Andromeda galaxy, our nearest major galaxy. Elliptical galaxies have smooth and almost featureless structures lacking arms and notable pockets of star formation.

Because they lack stellar nurseries and contain mostly old stars, elliptical galaxies are often considered “dead” when compared to their spiral relatives. However, astronomers have spotted signs of a population of young, blue stars at the center of Messier 110; it may not be “dead” yet.

Image Credit: NASA / ESA