What it is
The authors present the characteristics of interstellar comet 3I/ATLAS, discovered on 2025 July 1 by the Asteroid Terrestrial-impact Last Alert System (ATLAS). The comet has an eccentricity of about 6.1 and a velocity at infinity of about 57 km/s, indicating an interstellar origin. They obtained B, V, R, I, g, r, i and z photometry at Kottamia Astronomical Observatory, Palomar Observatory and Apache Point Observatory on 2025 July 2, 3 and 6, and measured the comet's colour indices and a spectral slope of 16.0 ± 1.9% per 100 nm. They estimate its dust cross-section within 10,000 km at 184.6 ± 4.6 km², assuming an albedo of 0.1; its coma has a full width at half-maximum of about 2.2 arcsec and an A(0°)fρ of 280.8 ± 3.2 cm. They estimate that 3I/ATLAS is ejecting micrometre to millimetre dust at about 0.01 to 1 m/s, with a mass loss of about 0.1 to 1.0 kg per second.
Why it matters
An eccentricity of about 6.1 and a speed far from the Sun of about 57 km/s indicate that comet 3I/ATLAS came from outside the solar system. The paper's arXiv version calls it the third known macroscopic interstellar object, after 1I/ʻOumuamua and 2I/Borisov. Within days of its discovery this paper measured its colours and a dusty coma, and estimated that it was losing about 0.1 to 1.0 kg of dust per second.
Underlined numbers link to their source. Every metric and quoted figure is listed under Sources and data below.
Filed underinterstellar object, comet, 3I/ATLAS, solar system, astronomy