Large Magellanic Cloud – Astronomy Now

The Sun expected to ride out a looming galactic merger

4 January 2019 Astronomy Now

A collision between the Milky Way and the Large Magellanic Cloud in about 1.5 billion years likely will re-energize the supermassive black hole lurking in our galaxy’s core.

Large Magellanic Cloud may be result of past galactic merger

18 September 2018 Astronomy Now

Computer simulations indicated the Large Cloud of Magellan may have merged with another luminous galaxy three to five billion years ago, a scenario that explains unusual stellar motions and ages.

Gaia takes a fingerprint of the Large Magellanic Cloud

3 May 2018 William Harwood

The European Space Agency’s Gaia spacecraft collected proper motion data for several million stars in the Large Magellanic Cloud, a satellite galaxy to the Milky Way, allowing astronomers to visualize its rotation in a unique fingerprint-like pattern.

Hubble spotlights irregular galaxy IC 3583

28 November 2016 Astronomy Now

This NASA/ESA Hubble Space Telescope image reveals a delicate blue group of stars — actually an irregular galaxy named IC 3583 — that sits some 30 million light-years away in the constellation of Virgo. This small galaxy is thought to be gravitationally interacting with one of its neighbours, the spiral Messier 90.

Major supercluster of galaxies found hidden by the Milky Way

17 November 2016 Astronomy Now

An international team of astronomers has discovered a previously unknown major concentration of galaxies in the constellation Vela, which they have dubbed the Vela supercluster. The gravitational attraction from this large mass concentration in our cosmic neighbourhood may have an important effect on the motion of our Local Group of galaxies.

Record-breaking extragalactic gamma-ray binary found

30 September 2016 Astronomy Now

Using data from NASA’s Fermi Gamma-ray Space Telescope and other facilities, an international team has found the first gamma-ray binary in another galaxy and the most luminous one ever seen. The dual-star system, dubbed LMC P3, contains a massive star and a crushed stellar core that interact to produce a cyclic flood of gamma rays.

South by Phil Hart

13 September 2016 Astronomy Now

The Southern Cross constellation of the Milky Way, visible in the southern sky creates a guiding light along Bucklands Lane in Central Goldfields Shire, Victoria, Australia.

Hubble peers into the maelstrom

5 September 2016 Astronomy Now

This NASA/ESA Hubble Space Telescope image shows a stellar nursery known as N159 — a maelstrom of glowing gas and dark dust within one of the Milky Way’s satellite galaxies, the Large Magellanic Cloud (LMC). N159 is located over 160,000 light-years away. It resides just south of the Tarantula Nebula, another massive star-forming complex within the LMC.

Hubble views supernova shrapnel

15 August 2016 Astronomy Now

Several thousand years ago, a star some 160,000 light-years away from us exploded, scattering stellar shrapnel across the sky. The aftermath of this Type Ia supernova is shown here in this striking image from the NASA/ESA Hubble Space Telescope. The exploding star was a white dwarf located in the Large Magellanic Cloud, a close neighbouring galaxy.

Hubble sees the shredded remains of a supernova

25 July 2016 Astronomy Now

This NASA/ESA Hubble Space Telescope image captures the remnants of a long-dead star. These rippling wisps of ionised gas, named DEM L316A, are the remains of an especially energetic Type Ia supernova located some 160,000 light-years away within one of the Milky Way’s closest galactic neighbours — the Large Magellanic Cloud (LMC).