Ghosts of ancient explosions live on in stars today

**Ghosts of ancient explosions live on in stars today
Image of a Type Ia supernova. Credit: Zwicky Transient Facility

When small, dense stars called white dwarfs explode, they produce bright, short-lived flares called Type Ia supernovae. These supernovae are informative cosmological markers for astronomers—for example, they were used to prove that the universe is accelerating in its expansion.

White dwarfs are not all the same, ranging from half of the mass of our sun to almost 50 percent more massive than our sun. Some explode in Type Ia ; others simply die quietly. Now, by studying the "fossils" of long-exploded , Caltech astronomers have found that early on in the universe, white dwarfs often exploded at lower masses than they do today. This discovery indicates that a white dwarf could explode from a variety of causes, and does not necessarily have to reach a critical mass before exploding.

A paper about the research, led by Evan Kirby, assistant professor of astronomy, appears in the Astrophysical Journal.

Near the end of their lives, a majority of stars like our sun dwindle down into dim, dense white dwarfs, with all their mass packed into a space about the size of Earth. Sometimes, white dwarfs explode in what's called a Type Ia (pronounced one-A) supernova.

It is uncertain why some white dwarfs explode while others do not. In the early 1900s, an astrophysicist named Subrahmanyan Chandrasekhar calculated that if a white dwarf had more than 1.4 times the mass of our sun, it would explode in a Type Ia supernova. This mass was dubbed the Chandrasekhar mass. Though Chandrasekhar's calculations gave one explanation for why some more massive white dwarfs explode, it did not explain why other white dwarfs less than 1.4 solar masses also explode.

Studying Type Ia supernovae is a time-sensitive process; they flare into existence and fade back into darkness all within a few months. To study long-gone supernovae and the white dwarfs that produced them, Kirby and his team use a technique colloquially called galactic archaeology.

Galactic archaeology is the process of looking for chemical signatures of long-past explosions in other stars. When a white dwarf explodes in a Type Ia supernova, it pollutes its galactic environment with elements forged in the explosion—heavy elements like nickel and iron. The more massive a star is when it explodes, the more will be formed in the supernova. Then, those elements become incorporated into any newly forming stars in that region. Just as fossils today give clues about animals that have long ceased to exist, the amounts of nickel in stars illustrates how massive their long-exploded predecessors must have been.

Using the Keck II telescope, Kirby and his team first looked at certain ancient galaxies, those that ran out of material to form stars in the first billion years of the universe's life. Most of the in these galaxies, the team found, had relatively low nickel content. This meant that the exploded white dwarfs that gave them that nickel must have been relatively low mass—about as massive as the sun, lower than the Chandrasekhar mass.

Yet, the researchers found that the nickel content was higher in more recently formed galaxies, meaning that as more time went by since the Big Bang, white dwarfs had begun to explode at higher masses.

"We found that, in the , white dwarfs were exploding at lower masses than later in the universe's lifetime," says Kirby."It's still unclear what has driven this change."

Understanding the processes that result in Type Ia supernovae is important because the explosions themselves are useful tools for making measurements of the universe. Regardless of how they exploded, most Type Ia supernovae follow a well-characterized relationship between their luminosity and the time it takes for them to fade.

"We call Type Ia supernovae 'standardizable candles." If you look at a candle at a distance, it will look dimmer than when it's up close. If you know how bright it is supposed to be up close, and you measure how bright it is at a distance, you can calculate that distance," says Kirby. "Type Ia supernovae have been very useful in calculating things like the rate of expansion of the universe. We use them all the time in cosmology. So, it's important to understand where they come from and characterize the white dwarfs that generate these explosions."

The next steps are to study elements other than nickel, in particular, manganese. Manganese production is very sensitive to the of the supernova that produces it, and therefore gives a precise way to validate the conclusions drawn by the content.

The paper is titled "Evidence for Sub-Chandrasekhar Type Ia Supernovae from Stellar Abundances in Dwarf Galaxies."

Explore further

Shining a new light on the evolution of supernovae

More information: "Evidence for Sub-Chandrasekhar Type Ia Supernovae from Stellar Abundances in Dwarf Galaxies," Evan Kirby et al., 2019, to appear in the Astrophysical Journal
Journal information: Astrophysical Journal

Citation: Ghosts of ancient explosions live on in stars today (2019, August 6) retrieved 18 August 2019 from
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Aug 06, 2019
Sounds like the 'pollution' of subsequent stellar generations by such 'metals' has had a subtle but far-reaching effect on internal dynamics, such the failing innards could cook for longer before collapse.

Um, been a long time since I studied such: where/how would such effects act ??

Aug 06, 2019
Star formation is one of the least comprehended phenomenon in astrophysics. Is there a general theory of star formation? No, there is not. There is a number of models based on computer simulations which include supersonic hydrodynamics with non-ideal MHD turbulence influenced by gravity. They include the line and continuum radiative processes of the energy transfer; a number of chemical processes with dissociation, recombination and ionization, with uncertain nomenclature of atoms and molecules, unknown magnetic fields and formation and destruction of dust particles. In addition there is macrophysics that is an environment in the molecular clouds, clumps and cores; inclusion in the multiple systems, collisions among stellar systems; jets and outflows; radiation pressure. https://www.acade...ormation

Aug 06, 2019
i thought the point of being a "ghost" was that you did not "live" on?

as to the subject of this article
it has been my (unsupported) opinion
that a common, though minor phenomena generally ignored as lacking in exciting discoveries?

is that of mundane ejection of stellar materials into ballistic orbits
yes, the major flash & bang of stars flaring & the novae & supernovae & hypernovae
are all well & good

however, it would seem reasonable to me, that much of the spectacle will, over millions, maybe billions of years?
get pulled back in by the main gravitational mass & recycled
no matter how far ejecta was originally flung away

momentum is not acceleration
no matter how politically correct it is to make that claim in altright fabulisms

not all of it returns of course
but enough material will eventually be infalling at random intervals for recycling
perhaps to trigger less violent repetitious cycles of flares or novae?

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