A weird star produced the fastest nova on record
This illustration shows an intermediate polar system, a type of two-star system that the research team thinks V1674 Hercules belongs to. A flow of gas from the large companion star impacts an accretion disk before flowing along magnetic field lines onto the white dwarf. Credit: Mark Garlick

The fastest nova ever recorded was observed by astronomer. Scientists were interested in an even more strange star. They may find answers to larger questions about the chemistry of our solar system, the death of stars and the evolution of the universe as a result of studying it.

The report was co-authored by Professor Sumner Starrfield from Arizona State University, Professor Charles Woodward from the University of Minnesota, and MarkWagner from The Ohio State University.

A nova is a burst of light from a star system. novas are created by a white dwarf and a companion star. The white dwarf draws matter from its companion which falls onto it. A burst of energy is created by the white dwarf's heat. The matter is shot away at high speeds and we can see it.

The nova fades over time. The nova V1674 Hercules burst so bright that it was visible to the naked eye, but it was faint once more. It was like someone was using a flashlight.

This nova is a precious study subject because of its rarity.

Starrfield, an astronomer in the School of Earth and Space Exploration at Arizona State University, said that the previous fastest nova was one we studied in 1991.

Other researchers discovered that Hercules' speed wasn't the only unusual trait. The light and energy it sends out is very loud.

Observers can see the wobble in both light waves and X-rays. The nova is still showing its wobble a year after it exploded. Starrfield and his colleagues have been studying it.

The head of science at the Large Binocular Telescope Observatory, which is being used to observe the nova, says that the most unusual thing is that it was visible before the eruption. The periodicity that you would see over that range of brightness is a mystery that people are trying to wrestle with.

The team noticed something strange as they monitored the nova explosion, which may be due to the position of the white dwarf and its companion star.

novae can tell us important information about our solar system and the universe as a whole, despite the fact that the fastest nova is flashy.

During a nova explosion, a white dwarf collects and changes matter in the surrounding space. The cycle of matter in space is important. New stellar systems will be formed by the materials ejected by novae. Earth is more than a lump of carbon thanks to events like these.

Starrfield says they are trying to figure out how the solar system formed. One thing that we're going to learn from this nova is how much lithium was produced. We're pretty sure that a lot of thelithium that we have on the Earth was produced by these types of explosions.

A white dwarf star can gain mass if it doesn't lose all of its collected matter during a nova explosion. The white dwarf could create a type 1a supernova, which is one of the brighter events in the universe, if this were to happen. Standard candles are what type 1a supernovas are known for.

We can see standard candles at great distances. Woodward says we can ask questions about how the universe is speeding up or how the three-dimensional structure of the universe is changing. One of the reasons we study these systems is because of this.

novae can tell us more about how stars evolve to their deaths, a process that is not well understood. Scientists can see nuclear physics in action in living laboratories.

The nova surprised the world. An amateur astronomer from Japan discovered it and reported it to scientists.

The field of astronomy is becoming more important with the help of citizen scientists. Even though it is too faint for other types of telescopes to see, the team is still able to monitor the nova thanks to the Large Binocular Telescope and its other equipment.

They will investigate the cause of the outburst, the processes that led to it, the reasons for its record-breaking decline, and the cause of its bright light.

More information: Research Notes of the American Astronomical Society (2022). DOI: 10.3847/2515-5172/ac779d