Around 15,000 years ago a star 20 times more massive than our Sun dramatically exploded in a region of space within the constellation Cygnus the Swan.
Since then the shockwave and expanding envelope of ejected stellar material and ionised gas has been racing apart, creating a nebulous structure over 130 light years across. This image, captured by Katie Hughes, from her home in Loch Lomond, is all that remains of this event (a supernova remnant) in visible light.
Thank you very much for sharing the stunning image Katie. Katie has recently started an Instagram page with more of her images. Please visit it here.
Some interesting new information has emerged on Betelgeuse, the red supergiant that marks the left ‘armpit’ of Orion the Hunter.
1. It’s still burning Helium in its core so unlikely to go supernova until around 100,000 years.
2. It’s not as massive as previously thought. Earlier studies had shown its radius would extend to the orbit ofJupiter if placed in our solar system. This new data suggests its real radius is 60% of this.
3. It’s closer to Earth than previously measured, at 530 light years. This is 25% closer than we previously thought.
New data published in the Astrophysical Journal. Further reading here.
See a supernova explosion in a distant galaxy over 50 million light years away.
Berto Monard witnessed Supernova 2015F in spiral galaxy NGC 2442 in March 2015, although the actual event happened 50 million years ago, long before human beings inhabited planet Earth.
Supernovae like this produce so much light energy they can briefly out shine the accumulated light from the entire galaxy. For this reason they can be witnessed even with moderately sized back garden telescopes, if you’re lucky enough to be pointing in the right direction at the right time!
Video Credit & Copyright: Changsu Choi & Myungshin Im (Seoul National University)
Source: Robert Nemiroff (MTU) & Jerry Bonnell (UMCP)
This is an amazing composite image of the Crab Nebula supernova remnant. It shows the neutron star at the center, superimposed over the shockwave nebula (whose outline can be observed dimly in a decent telescope).
This is what happens to high mass stars when they run out of fuel. The atmosphere of the star suddenly collapses inward and dramatically rebounds off the compressed neutron core.
Conservation of angular momentum makes the neutron star spin rapidly (a pulsar) and the rest of the star’s atmosphere expands into space releasing huge quantities of energy (a supernova).
This particular supernova was observed and recorded by Chinese astronomers in 1054 AD as a ‘guest star’, in the constellation Taurus. It remained visible as a naked eye star for over a year before fading.
I can’t get over how much dimmer Betelgeuse in Orion appears at the moment. To my eye Aldebaran (a red giant) in Taurus now appears obviously brighter.
This was an image taken last winter.
Orion image from winter 2019
Many click bait astronomy articles have surfaced claiming the star might be dimming due to its impending collapse and rebound as a supernova, but Betelgeuse is a known variable star and similar changes in its brightness have been noted in the past, although recent changes appear to deviate from established patterns.
Unusual gravitational waves have also been detected in the vicinity of the red supergiant, adding to the sense of mystery. It’s important to note that these waves are merely in the vicinity, so could easily be generated by countless other sources behind Betelgeuse.
Still, it’s fun to speculate about the possibility of witnessing a relatively close supernova event in our lifetime. The last two major naked eye supernovas were recorded in 1572 and and 1054, in Taurus (the Crab nebula) and Cassiopeia (Tycho Brahe supernova). Both generated enough luminosity to be visible in daylight for several weeks, and shone as new ‘guest stars’ for around a year or so before fading.
Some work published by Dolan in 2016 estimated the impact of a Betelgeuse supernova on Earth and found it to be negligible. At 500 light years distance the residual energy of the vastly expanded shockwave would be exponentially diminished as it passed Earth. However the brightness predicted would be magnitude -12.4, making such an event more luminous than a full Moon!
For the mathematically motivated I enclose an extract from his calculations below.
The main constellations were visible over the Merkinch nature reserve in the west of Inverness, and even a hint of Milky Way.
We had a great evening at the Merkinch Urban Astronomy gathering tonight. Big thanks to Dr Anthony Luke for delivering a fascinating talk on the chemistry of stars and supernovas. We learnt all about the synthesis of elements and compounds forged in the heart of stars.
Afterwards we were rewarded with clear skies, so I led a group up to the nature reserve for a blustery stargazing session over the Beauly Firth.
Overlooking the water we had lovely views of Orion, the Pleiades and even a hint of the Milky Way and the Andromeda galaxy.
The next event is an Aurora Special on Feb 20th with guest Graham Bradshaw.
In 1054AD Chinese astronomers recorded a bright new star suddenly appear in the constellation Taurus the bull. It brilliantly out shone all other stars and was visible in broad daylight. After a year or so its light faded and it vanished.
The event was a supernova explosion – the dramatic explosion of a massive star. Today we can see the remnants left behind from this violent event – the Crab Nebula. An expanding shockwave of recycled stellar material. The above amazing image is from the Hubble space telescope.
You can see the Crab Nebula in a modestly sized amateur telescope, and as always the darker the skies the more detail you’ll see. With a 150mm scope or larger you should be able to trace out the overall mottled shape of the nebula. Use averted vision and see if you can pick out extra detail and structure.
Finding the Crab is relatively straightforward as it sits just beside the lowest horn of the constellation Taurus the bull, which sits above and right of Orion during evening skies at the moment.