3I ATLAS (2025 N1): The third interstellar object within our solar system


(under construction)
by Wm. Robert Johnston
last updated 17 May 2026


Discovery and designation

A comet was discovered by the Asteroid Terrestrial-impact Last Alert System (ATLAS) in Chile and reported on 1 July 2025, temporarily designated A11pl3Z. Within 6 hours of the ATLAS detection, additional observations were identified from 28-29 June 2025 by the Zwicky Transient Facility (ZTF), sufficient to show that the orbit was extremely hyperbolic (Seligman et al., 2025). Follow up observations were conducted during the first 24 hours from many facilities, plus additional pre-discovery observations were found with the earliest being from ZTF on 14 June 2025. On 2 July the Minor Planet Center assigned it the designation 3I/ATLAS as the third interstellar object (after 1I/'Oumuamua and 2I/Borisov) plus the cometary designation C/2025 N1 (ATLAS). Pre-discovery observations were later identified from as early as 15 May 2025. At the time of discovery 3I/ATLAS was 4.5 AU from the Sun, 3.5 AU from the Earth, and had a magnitude of ~17.8.


Orbit and ephemeris (MPC, 2025)

perihelion distance q:
eccentricity e:
inclination i:
ascending node Ω:
longitude of perihelion ω:
time of perihelion Tp:
Epoch:
absolute magnitude H:
data arc:
1.3745928 AU
6.2769203
175.11669°
322.27219°
127.79317°
2025 Oct 29.21095
2025 May 5.0
-
19 days (2025 Jun 14-Jul 2), 122 obs.

Orbit and ephemeris (JPL, 2026)

perihelion distance q:
eccentricity e:
inclination i:
ascending node Ω:
longitude of perihelion ω:
mean anomaly M:
time of perihelion Tp:
Epoch:
nongravitational parameter A1:
nongravitational parameter A2:
nongravitational parameter A3:
total magnitude M1:
total magnitude slope K1:
data arc:
1.3564811 ± 0.0000038 AU
6.141351 ± 0.000025
175.116457 ± 0.000019°
322.169609 ± 0.000071°
128.02287 ± 0.00010°
818.2202 ± 0.0029°
2025 Oct 29.495263 ± 0.000051
2026 Feb 19.0
(53.2 ± 1.2) x 10-9 AU/day2
(11.5 ± 2.1) x 10-9 AU/day2
(-6.85 ± 0.18) x 10-9 AU/day2
12.5 ± 0.9
4.5
280 days (2025 May 15-2026 Feb 19), 782 obs.

datemagnitudedistance to
Sun (AU)
distance to
Earth (AU)
notes
2013 Jan 0133.20157.990158.950
2014 Jan 0132.87145.748146.706
2015 Jan 0132.51133.505134.463
2016 Jan 0132.11121.261122.218
2017 Jan 0131.67108.982109.942
2018 Jan 0131.1896.73397.693
2019 Jan 0130.6384.48085.440
2020 Jan 0129.9972.22273.181
2021 Jan 0129.2259.92160.884
2022 Jan 0128.2947.64448.607
2023 Jan 0127.0735.35036.315
2024 Jan 0125.3323.03324.001
2024 Jul 0123.8316.87615.874
2025 Jan 0122.2510.63811.618
2025 Jan 1522.0610.16311.132
2025 Feb 0121.829.58610.466
2025 Feb 1521.599.1119.860
2025 Mar 0121.348.6369.210
2025 Mar 1521.068.1618.523
2025 Apr 0120.687.5847.658
2025 Apr 1520.347.1096.935
2025 May 0119.916.5686.116
2025 May 1519.506.0945.423earliest pre-discovery observation
2025 Jun 0118.975.5204.640
2025 Jun 1118.645.1844.220crosses Jupiter's orbit inbound
2025 Jun 1418.545.0834.102earliest pre-discovery observation used for announcement
2025 Jun 1518.515.0504.063
2025 Jul 0117.974.5143.507discovery
2025 Jul 1517.514.0493.127
2025 Aug 0116.993.4922.811
2025 Aug 1516.603.0422.661
2025 Sep 0116.162.5152.575
2025 Sep 1515.792.1102.542
2025 Oct 0115.341.7092.500
2025 Oct 0315.281.6652.492closest approach to Mars (0.194 AU)
2025 Oct 1514.961.4562.429
2025 Oct 2914.721.3562.311perihelion
2025 Nov 0114.691.3592.280
2025 Nov 0314.681.3662.257closest approach to Venus (0.649 AU)
2025 Nov 0714.671.3912.211brightest as seen from Earth
2025 Nov 1514.691.4842.110
2025 Dec 0114.861.8001.911
2025 Dec 1515.092.1661.804
2025 Dec 1915.182.2801.797closest approach to Earth
2026 Jan 0115.582.6671.873
2026 Jan 1516.173.1062.144
2026 Feb 0116.993.6552.699
2026 Feb 1517.654.1153.287
2026 Mar 0118.264.5813.949
2026 Mar 1518.805.0494.654
2026 Mar 1718.885.1174.756closest approach to Jupiter (0.360 AU)
2026 Mar 2018.985.2174.911crosses Jupiter's orbit outbound
2026 Apr 0119.395.6215.535
2026 Apr 1519.826.0946.260
2026 May 0120.256.6357.070
2026 May 1520.587.1097.748
2026 Jun 0120.947.6858.521
2026 Jun 1521.208.1609.106
2026 Jul 0121.478.7039.712
2026 Jul 1521.679.17810.185
2026 Aug 0121.909.75510.687
2026 Aug 1522.0610.23011.044
2026 Sep 0122.2410.80711.416
2026 Oct 0122.5211.82411.955
2026 Nov 0122.7712.87612.469
2026 Dec 0123.0313.89313.078
2027 Jan 0123.3114.94313.961
2028 Jan 0125.8627.28026.299
2029 Jan 0127.4339.61438.634
2030 Jan 0128.5551.89550.916
2035 Jan 0131.79113.223112.244
2040 Jan 0133.58174.462173.483
2045 Jan 0134.83235.697234.719
2050 Jan 0135.78296.896295.918


Confirmation as interstellar in origin

3I/ATLAS is the most hyperbolic object yet observed with an eccentricity of 6.14; its velocity relative to the Sun prior to significant influence of the Sun's gravity was 57.9 km/s. The hyperbolic nature was confirmed within hours of discovery (Seligman et al., 2025).


Follow-up observations

3I/ATLAS will come no closer than 1.8 AU to the Earth, making telescopic observations challenging. However, its path is close to the ecliptic and it passed only 0.19 AU from Mars on 3 October 2025 and will pass only 0.36 AU from Jupiter on 16 March 2026. Consequently several planetary probes have been and will be tasked to make observations (though obviously with much smaller telescopes than ground-based ones).


Cometary activity

Faint activity was visible in images from the Canada-France-Hawaii Telescope (CFHT) on 2 July with an elongated coma visible in images from the European Southern Observatory Very Large Telescope (ESO VLT) on 4 July (Seligman et al., 2025).


Size

The nucleus of 3I/ATLAS itself is unresolved. Hubble Space Telescope observations suggest its diameter is between 0.44 and 5.6 km (Jewitt et al., 2025). The lower limit is set by assumptions about the volatile which is driving coma formation and the upper limit by an assumed cometary albedo and coma brightness distribution; the actual size is more likely towards the lower limit. Estimates based on observed non-gravitational acceleration suggest a diameter between 0.82 and 1.05 km (Forbes and Butler, 2025), using assumptions regarding outgassing asymmetry and density (0.5 g/cm3 assumed).

De la Fuente Marcos et al. (2025) report a rotation period of 16.79 ± 0.23 h and an amplitude of ~0.2 magnitude, which suggests a relatively small elongation of >1.2 for the nucleus (though this depends on how much of 3I's brightness is from the dust coma rather than the nucleus).


References

--articles and preprints on 3I/ATLAS (from newest to oldest; arXiv posting date in parentheses)

--other items on 3I/ATLAS (from newest to oldest)

--Minor Planet Center releases on 3I/ATLAS

--International Astronomical Union releases on 3I/ATLAS

--background articles and data sets


Comments? Questions? Corrections? Contact me.
Last modified 17 May 2026.
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