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Dusty construction explains close to vanishing of faraway star

August 23, 2025
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Dusty structure explains near vanishing of faraway star
Schematic diagrams of the potential configurations mentioned for ASASSN-24fw. They don’t seem to be drawn to scale. The yellow circle is the F star, the darkish pink circle is the proposed M dwarf companion and the sunshine brown sphere is the optically skinny circumstellar mud. Credit score: The Open Journal of Astrophysics (2025). DOI: 10.33232/001c.143105

Stars die and vanish from sight on a regular basis, however astronomers have been puzzled when one which had been steady for greater than a decade nearly disappeared for eight months.

Between late 2024 and early 2025, one star in our galaxy, dubbed ASASSN-24fw, dimmed in brightness by about 97%, earlier than brightening once more. Since then, scientists have been swapping theories about what was behind this uncommon, thrilling occasion.

Now, a world group led by scientists at The Ohio State College might have give you a solution to the thriller. In a brand new examine not too long ago printed in The Open Journal of Astrophysics, astronomers recommend that as a result of the colour of the star’s gentle remained unchanged throughout its dimming, the occasion wasn’t attributable to the star evolving in a roundabout way, however by a big cloud of mud and fuel across the star that occluded Earth’s view of it.

“We explored three totally different situations for what could possibly be happening,” stated Raquel Forés-Toribio, lead creator of the examine and a postdoctoral researcher in astronomy at Ohio State. “Proof suggests it’s possible that there’s a cloud of mud within the type of a disk round it.”

ASASSN-24fw is an F-type star—a star that is a bit more huge than our solar and about twice as huge—and is positioned about 3,000 light-years away from Earth. Researchers estimate that the cloudy disk it is surrounded by is about 1.3 astronomical units (AU) throughout, even greater than the space between the solar and our planet. (One AU is the space between the middle of Earth and the middle of the solar.)

Researchers recommend this disk can also be possible made up of huge clusters of carbon or water ice shut in dimension to a big grain of mud discovered on Earth. This materials is analogous sufficient to planet-forming disks that learning it might give astronomers novel insights into stellar formation and evolution.

But these findings alone do not clarify the entire system’s abnormalities, stated Forés-Toribio. As an alternative, researchers assume {that a} smaller, cooler star may additionally orbit ASASSN-24fw, which might make it a hidden binary system.

“At this second, with the info that we now have, what we suggest is that there needs to be two stars collectively in a binary system,” stated Forés-Toribio. “The second star, which is far fainter and fewer huge, could also be driving the modifications in geometry resulting in the eclipses.”

Whereas dimming techniques just like the one the group noticed are uncommon, this one-in-a-million eclipsing was particularly dramatic, stated Chris Kochanek, co-author of the examine and a professor of astronomy at Ohio State, as even when researchers looked for related objects, they could not discover one which match the identical precise sample.

“We have been hoping to seek out some similarities and we did not actually discover very many, which is fascinating in and of itself,” stated Kochanek. “However the hope is, as we discover extra sooner or later, some patterns may finally be revealed.”

The system was found as a part of the All-Sky Automated Survey for Supernovae (ASAS-SN) challenge, a community of small telescopes that monitor all the seen night time sky. Since its institution greater than a decade in the past, ASAS-SN has collected about 14 million photographs and counting of the cosmos.

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“The universe’s capability to shock us is steady,” stated Krzysztof Stanek, one other co-author of the examine and a professor of astronomy at Ohio State. “Even with small telescopes on the bottom and massive telescopes in area, each time we get a brand new functionality, we nonetheless uncover new issues.”

In accordance with the group, the ASASSN-24fw system possible experiences an eclipse about as soon as each 43.8 years, with the subsequent one not anticipated to happen till round 2068. Whereas some members of the group do not count on to be round to check that occasion, they hope that the work they depart in cultivating these long-term sky surveys provides future scientists a basis to make all kinds of recent, thrilling discoveries.

“We wish our knowledge to be accessible 100 years from now, even when we aren’t round,” stated Stanek. “The primary level of ASAS-SN is, if one thing occurs within the sky, we’ll have historic knowledge for it.”

Within the meantime, the group needs to utilize bigger telescopes just like the James Webb House Telescope and the ground-based Massive Binocular Telescope Observatory to make extra full observations of the system because it returns to full brightness.

“This examine is a very fascinating instance of a broader class of nonetheless very unusual objects,” stated Stanek. “We study extra about astrophysics once we discover issues which might be uncommon, as a result of it pushes our theories to the take a look at.”

Different Ohio State co-authors embrace Brayden JoHantgen, Michael Tucker, Lucy Lu and Dominick Rowan, in addition to scientists at Boston College, College of Hawai’i, Carnegie Observatories, College of Vienna, Florida State College, The College of Melbourne, College of California, Santa Cruz and Ball State College.

Extra data:
Raquel Forés-Toribio et al, ASASSN-24fw: An 8-month lengthy, 4.1 magazine, optically achromatic and polarized dimming occasion, The Open Journal of Astrophysics (2025). DOI: 10.33232/001c.143105

Supplied by
The Ohio State College


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