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Nova Reticuli 2020 bursts into the southern skies

The blast from a white dwarf in the Milky Way has brought it briefly to naked-eye visibility.
RELATED TOPICS: OBSERVING | STARS
GKPersei1901
GK Persei 1901, a classical nova discovered in 1901, has undergone several outbursts in subsequent years. Surrounding it is the Firework Nebula, the expanding remnants of gas and dust blown away by the explosions. A similar nova, Nova Reticuli 2020, has been spotted in the Southern Hemisphere.
Adam Block/Mount Lemmon SkyCenter/University of Arizona
Southern Hemisphere observers are in for a transient treat: There’s now a naked-eye nova in the sky.

Nova Reticuli 2020 was spotted by veteran comet hunter Robert McNaught from Coonabarabran, Australia, on July 15. It’s currently visible around magnitude 5, near the bright stars Alpha (α) and Gamma (γ) Doradus. You can pinpoint it by looking roughly 5° west of magnitude 3.3 Alpha and 4.25° southwest of magnitude 4.3 Gamma.

The nova should appear as a new star in the sky where you don’t expect to see one. If you can’t spot it unaided or live in a light-polluted area, binoculars or a small telescope should easily bright it into view.
NovaReticuli2020Finder
Nova Reticuli 2020
You can find Nova Reticuli 2020 near two bright stars in the constellation Dorado, visible in the Southern Hemisphere.
Alison Klesman (via TheSkyX)

A classical nova

Following the discovery, quick follow-up work by additional astronomers indicates the event is a classical nova, which occur in binary systems housing a white dwarf (the remnant of a Sun-like star) and a main sequence, hydrogen-burning star. If the two are in a tight enough orbit, the white dwarf can pull material off its companion. This transferred mass — mainly hydrogen — piles onto the white dwarf’s surface. Eventually, enough accumulates that the temperature and pressure at the surface rise, sparking a thermonuclear reaction. The reaction causes the built-up hydrogen to rapidly undergo fusion into heavier elements, releasing immense amounts of energy in a blast we see from Earth as a nova.

This is a bit like what happens during a Type Ia supernova, but there’s a key difference: Type Ia supernovae destroy their white dwarf progenitors, while classical novae do not. That’s because the runaway reaction happens within the white dwarf during a supernova, blasting it to bits. During a nova, the reaction only happens on the white dwarf’s surface, leaving the rest of the star intact. So, a Type Ia supernova can only happen once, but a classical nova can reoccur numerous times.

Observers have noted that Nova Reticuli 2020’s position in the sky is close to a previously discovered object, MGAB-V207, which astronomers classify as a VY Scl-type cataclysmic variable — meaning it has previously undergone sudden drops in brightness that astronomers associate with episodes of mass transfer from a companion to a white dwarf. According to an Astronomer’s Telegram, the coincident positions, coupled with the follow-up observations indicating that this particular outburst is a classical nova, suggest Nova Reticuli 2020 may be the third ever classical nova observed in a star system previously known to contain a white dwarf.  

If you’re a Southern Hemisphere observer interested in adding your data to the mix, you can submit observations to the American Association of Variable Star Observers using the object name MGAB-V207 or N RET 2020.



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