SUBSCRIBE NOW

SIGHT

Be informed. Be challenged. Be inspired.

Introducing Janus, the exotic “two-faced” white dwarf star

Washington DC, US
Reuters

Some people are two-faced, figuratively speaking of course. The ancient Roman god Janus was two-faced, literally – with one looking forward and another backward, representing transitions and duality. But a two-faced star? Yes, indeed.

Scientists have observed a white dwarf star – a hot stellar remnant that is among the densest objects in the cosmos – that they have nicknamed Janus owing to the fact it has the peculiar distinction of being composed of hydrogen on one side and helium on the other.

An artist's concept shows the two-faced white dwarf star nicknamed Janus.

An artist’s concept shows the two-faced white dwarf star nicknamed Janus. The blue-tinted dead cinder of a star, which was once a star like our sun, is composed primarily of hydrogen on one side and helium on the other (the hydrogen side appears brighter). On the helium side, which appears bubbly, convection has destroyed the thin hydrogen layer on the surface and brought up the helium underneath. PICTURE: K Miller, Caltech/IPAC/Handout via Reuters/File Photo

“Janus is the Roman god with two faces, so we thought it was very appropriate. Moreover, Janus is the god of transition, and the white dwarf might be currently transitioning from having an atmosphere made of hydrogen to one made of helium,” said Ilaria Caiazzo, a Caltech postdoctoral fellow in astrophysics and lead author of the study published last week in the journal Nature.

The star is located in our Milky Way galaxy about 1,300 light years from Earth in the direction of the Cygnus constellation. A light year is the distance light travels in a year, 9.5 trillion kilometres.

Janus is fairly massive for a white dwarf, with a mass 20 per cent larger than that of our sun compressed into an object with a diameter half that of Earth. It rotates on its axis every 15 minutes – very fast considering these stars usually rotate every few hours to a few days.

“White dwarfs form at the very end of a star’s life. About 97 per cent of all stars are destined to become white dwarfs when they die,” Caiazzo said. 

“Our sun, for example, is currently burning hydrogen into helium in its core. When the hydrogen in the core is depleted, the sun will start burning helium into carbon and oxygen. When the helium also is gone from the center, the sun will eject its outer layers into space in an event called a planetary nebula and the core will slowly contract and become a white dwarf,” Caiazzo added.



The good news for Earthlings is that it should be five billion years before any of that happens to our sun. 

Janus was spotted using the Zwicky Transient Facility at Caltech’s Palomar Observatory near San Diego, with subsequent observations made by other ground-based telescopes.

After a white dwarf forms, its heavier elements are thought to sink to the star’s core while its lighter elements – hydrogen being the lightest, followed by helium – float to the top. This layered structure is believed to be destroyed at a certain stage in the evolution of some white dwarfs when a strong mixing blends the hydrogen and helium together.

Janus may represent a white dwarf in the midst of this transitional blending process, but with the puzzling development of one side being hydrogen while the other side is helium. 


We rely on our readers to fund Sight's work - become a financial supporter today!

For more information, head to our Subscriber's page.


The researchers suspect that its magnetic field may be responsible for this asymmetry. If the magnetic field is stronger on one side than the other, as is often the case with celestial objects, one side could have less mixing of elements, becoming hydrogen heavy or helium heavy.

“Many white dwarfs are expected to go through this transition, and we might have caught one in the act because of its magnetic field configuration,” Caiazzo said.

Janus is not the only exotic white star known. Caiazzo was part of a research team that in 2021 reported on one with a petite diameter slightly larger than Earth’s moon that boasted the greatest mass and littlest size of any known white dwarf.

“Every time we look at stars in a different ways, we are bound to be surprised and even baffled sometimes,” Caiazzo said. “Stellar phenomenology is extremely rich, and no two stars are the same if looked at closely enough.”

Donate



sight plus logo

Sight+ is a new benefits program we’ve launched to reward people who have supported us with annual donations of $26 or more. To find out more about Sight+ and how you can support the work of Sight, head to our Sight+ page.

Musings

TAKE PART IN THE SIGHT READER SURVEY!

We’re interested to find out more about you, our readers, as we improve and expand our coverage and so we’re asking all of our readers to take this survey (it’ll only take a couple of minutes).

To take part in the survey, simply follow this link…

Leave a Reply

Your email address will not be published. Required fields are marked *

For security, use of Google's reCAPTCHA service is required which is subject to the Google Privacy Policy and Terms of Use.