3I/ATLAS Rotates On A 7.1 Hour Clock After Perihelion, According to New Analysis

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Images of 3I/ATLAS from January 13, 2026, shown in grayscale (left), false color (center), and Larson–Sekanina filtered views (right), revealing a prominent sunward anti-tail jet. As the object nears opposition on January 22, 2026, the anti-sunward jet is expected to fade while the anti-tail points toward Earth. (Image credit: Toni Scarmato and Antonio Brosio. Used for editorial purposes under 17 U.S.C. §107.)

KEY FINDINGS

  • When 3I/ATLAS passed closest to the Sun in October 2025, astronomers anticipated that the encounter could dramatically alter how the object behaves.
  • Perihelion passages often reshape comets and interstellar visitors, sometimes changing their rotation, triggering new jets, or destabilizing their structure.
  • According to new analysis published by Avi Loeb, 3I/ATLAS appears to have emerged from that encounter spinning at nearly the same pace — about once every seven hours.

Avi Loeb’s latest findings suggest the interstellar object’s spin remained stable through its closest solar encounter, raising new questions about its internal structure and jet behavior.

[USA HERALD]In a recent Medium post, Loeb reports that post-perihelion observations of 3I/ATLAS indicate a rotation period of approximately 7.1 hours, based on two independent observational techniques. The findings are drawn from a new paper co-authored with astronomer Toni Scarmato and rely on both jet orientation measurements and brightness variability.

One method tracks periodic changes in the orientation of jets emitted from the object as it rotates. The second examines rhythmic variations in the object’s overall brightness, which includes light scattered by the surrounding coma and jet structures rather than the nucleus itself.

Using images captured by the Hubble Space Telescope between November 20 and December 27, 2025, the researchers measured subtle “wobbles” in the position angle of the anti-sunward jet. Those wobbles, shifting by roughly ±20 degrees, repeated with a period of about 7.2 hours.

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Separately, brightness data collected between December 9 and December 22, 2025 from the MPC L92 observatory in Calabria, Italy showed periodic fluctuations of roughly ±30 percent. That signal yielded a nearly identical period of 7.136 hours.

According to Loeb, the close agreement between the two methods supports a post-perihelion rotation period of about seven hours, suggesting that the object’s spin rate did not undergo a major change during its closest approach to the Sun on October 29, 2025.

What did change, however, was how that rotation manifests observationally.