It is NGC 520, and was discovered by William Herschel in 1784. What Herschel didn’t know is that ultimately this object would be classified as a peculiar galaxy.

NGC 520 glows softly at magnitude 11.4 and measures 4.6′ by 1.9′. Through a 6-inch telescope at low power, you’ll think you’re looking at an edge-on spiral.

The picture below is NGC 520, a pair of interacting galaxies which started their collision 300 million years ago in the constellation Pisces. It is about 100 million light-years away and 100,000 ...

The galaxy sits in a sweet spot that allows astronomers to study it in ways that can't be applied to even our own Milky Way ...

This portrait from the NASA/ESA Hubble Space Telescope puts the nearby galaxy NGC 4449 in the spotlight. The galaxy is ...

Space. See 4K Imagery Of Colliding Galaxies From Siena Galaxy Atlas. Posted: July 30, 2024 | Last updated: July 30, 2024. See amazing views of colliding galaxies NGC 520 and barred galaxy IC 4212 ...

The galaxy NGC 4666 takes pride of place at the centre of this new image, made in visible light with the Wide Field Imager on the MPG/ESO 2.2-metre telescope at the La Silla Observatory in Chile.

Galaxy NGC 7292 is mesmerizing proof that there’s always more to see beyond a first glance. This article was originally published on June 16, 2023. Learn Something New Every Day.

NGC 520 was discovered by William Herschel in 1784 and is one of the largest and brightest galaxies in the Siena Galaxy Atlas. ... This galaxy appears face-on from Earth, ...

NGC 520 is one of the largest and brightest galaxies in the Siena Galaxy Atlas. It is made of two disk galaxies that will eventually merge together to form one massive system.

NGC 520’s unique shape is a result of a two-galaxy collision – one galaxy’s dust lane can be seen easily in the foreground. Our own galaxy – the Milky Way – will collide with the ...

It is NGC 520, and was discovered by William Herschel in 1784. What Herschel didn't know is that ultimately this object would be classified as a peculiar galaxy.