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Source: PreprintarXiv1 source

Two Telescopes Track Down an Asteroid That Hides in the Sun's Glare

Space

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Two enclosures of ESO's Very Large Telescope on a rocky ridge at Cerro Paranal in Chile, silhouetted against a deep blue twilight sky with an orange band of afterglow along the horizon.
ESO's Very Large Telescope stands on Cerro Paranal in Chile, where the asteroid's colors were measured in October 2026. An object on an orbit like this one can be caught only low in the sky, in the short window after sunset or before sunrise (illustrative)."Twilight at Paranal (gerd huedepohl 10)" by G. Hüdepohl (atacamaphoto.com)/ESO, via Wikimedia Commons, CC BY 4.0

Two of the world's largest telescopes have re-found a small asteroid whose orbit lies entirely inside Earth's and measured the color of its surface, which most closely matches that of the basalt-like V-type asteroids. The authors say that is consistent with a fragment of a larger body that once melted.

The asteroid Vesta, a gray, heavily cratered body with a bulging, irregular outline, lit from the lower left against black space.
Vesta, the large main-belt asteroid whose basalt-rich surface gives the V-type class its name, seen by NASA's Dawn spacecraft on July 24, 2011. The colors measured for 2025 SC79 are closest to that class (illustrative). "Vesta in natural color (cropped)" by NASA / JPL / MPS / DLR / IDA / Björn Jónsson, via Wikimedia Commons, Public domain

2025 SC79 sits on the boundary between asteroids that stay inside Venus's orbit and those that reach beyond it: the far point of its orbit lies less than a thousandth of the Earth-Sun distance outside Venus's closest approach to the Sun. The authors write that objects near that line can show how asteroids cross between the two groups.

Such asteroids are hard to find. Because they never appear far from the Sun in the sky, they can only be seen low in twilight, where a bright sky and thick air near the horizon cut a survey's sensitivity. A 2026 count cited by the authors lists 37 inside Earth's orbit, and one inside Venus's.

Bryce T. Bolin of Eureka Scientific and colleagues recovered the asteroid with the Keck I telescope in Hawaii on Oct. 7, 2026, and measured its colors with the FORS2 camera on the Very Large Telescope in Chile later in October 2026. Assuming the surface reflects light like others of its class, they put the diameter at 0.379 km. A published model of how asteroids reach the inner solar system gives a combined 95.4% probability that this one escaped from the inner main belt. Their preprint, submitted to Astronomy & Astrophysics, has not been peer-reviewed, and the authors say spectroscopy is needed to confirm the classification.

The team also followed 10,000 slightly different orbits consistent with the data, 5 million years forward and back. Those orbits cross the Venus line in both directions, and in the forward runs 14.56% of them end in a collision with Venus: a statistic about where a cloud of possible orbits finishes over millions of years, not a forecast for 2025 SC79.

S. S. Sheppard discovered 2025 SC79 on Sept. 27, 2025, with the Dark Energy Camera on the Blanco telescope in Chile.

A white, faceted telescope dome standing alone on bare ground at Cerro Tololo in Chile under a night sky crossed by the band of the Milky Way.
The Blanco dome at Cerro Tololo in Chile. Its Dark Energy Camera picked up 2025 SC79 on Sept. 27, 2025, a year before the two bigger instruments found it again (illustrative). "Víctor M Blanco 4-meter Telescope (noirlab-tololo-02)" by CTIO/NOIRLab/NSF/AURA/D. Munizaga, via Wikimedia Commons, CC BY 4.0

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Two Telescopes Track Down an Asteroid That Hides in the Sun's Glare

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