3I-Atlas Comet

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Everything you need to know about 3I-Atlas

Here are all the major facts about 3I/ATLAS:

Discovered by the Asteroid Terrestrial‑impact Last Alert System (ATLAS) survey telescope in Rio Hurtado, Chile, on 1 July 2025 (while about 4.5 AU from the Sun).
Official designation: 3I/ATLAS, also known as C/2025 N1 (ATLAS).
The “3I” means it’s the third known interstellar object (“I” = interstellar) to pass through our Solar System. The prior two were 2I/Borisov (2019) and 1I/ʻOumuamua (2017).
Because of its path (see below) it is not bound to the Sun—just passing through.

It follows a hyperbolic orbit (eccentricity well above 1) — confirming it came from outside our Solar System.
Closest approach to the Sun (perihelion): about 1.4 AU (~130 million miles / ~210 million km) around 30 October 2025.
Closest approach to Earth: about 1.8 AU (~270 million km) — so no threat whatsoever.
Velocity: Very fast. E.g., reported ~ 58 km/s relative to Sun, or ~130,000 mph in some reports.
Inclination & origin: Its path is unusual: retrograde orbit, low inclination relative to ecliptic (~5°) and appears to originate from the direction of the constellation Sagittarius, suggestive of coming from the Milky Way’s thick disk.

Classed as a comet (because of detected coma/dust tail) rather than a bare asteroid.
Chemistry: Very unusual compared to typical Solar System comets:

The James Webb Space Telescope (JWST) and other instruments observed a coma dominated by CO₂, with a CO₂/H₂O mixing ratio of ~ 8 ± 1 — among the highest seen in any comet.
Also detected: H₂O, CO, OCS, water ice and dust.
Polarimetric measurements indicate a “deep and narrow negative polarisation branch … unlike any known solar-system comet”.

Size: Estimates are uncertain. Some media reports claim “~7 miles (~11 km) wide” making it the largest interstellar object yet. But those are preliminary and speculative.
Activity: Showed outgassing/dust emission even when still far from Sun.

Opportunity: Because it comes from outside our Solar System, 3I/ATLAS gives scientists a rare chance to study material formed around another star.
Unusual composition means it may have formed in an environment very different from our Solar System (e.g., near a CO₂ ice line, or exposed to higher radiation). The high CO₂ suggests “exposed ices” or different formation region.
It expands the diversity of known interstellar objects — things we thought we knew about comets may be too Solar-System-centric.

It was visible to ground-based telescopes through September 2025 before it moved too close to Sun (for safe observation).
Expected to re-emerge after the Sun-occlusion side in early December 2025 for renewed observations.
It will leave our Solar System and continue into interstellar space, never to return.

Because its chemistry is odd, some speculation exists (e.g., by Avi Loeb) that it might be an artificial object (alien probe?) rather than purely natural. Most scientists remain skeptical.
The true size, nucleus structure, and detailed composition remain uncertain — data still being analysed.
The exact origin (which star system or region) is unknown — though “thick disk of Milky Way” is a hypothesis.
Future spacecraft interception has been proposed, but none currently planned for certain.

3I/ATLAS is a rare visitor from outside our Solar System, only the third confirmed.
It’s showing weird chemistry (CO₂-rich coma) unlike most comets we know.
It poses no danger to Earth.
It gives us a glimpse of material from another star system — a bit of cosmic “foreign delegation”.
Many details still uncertain; lots of excitement because novelty = research gold.

Parameter	Value(s)	Notes & caveats
Apparent magnitude	~ 14.2 on 14 Sept 2025.	That’s the total (nucleus + coma). Not naked-eye.
Absolute visual magnitude (H)	~ 12.5 ± 0.3 from TESS pre-discovery.	Assumes certain albedo; real size still very uncertain.
Nucleus diameter estimate (upper limit)	≤ 5.6 km (≈3.5 miles) from Hubble Space Telescope at 21 July 2025.	“Upper limit” means it could be much smaller.
Nucleus diameter estimate (lower plausible)	≥ 0.32 km (≈320 m) - estimates state range from 0.32 km to 5.6 km.	Because the coma masks the nucleus.
Dust-mass loss rate	~ 6-60 kg/s depending on particle size (1-100 µm).	Derived from Hubble coma models; depends strongly on assumptions.
Dust-production index with heliocentric distance	n = 3.8 ± 0.3 across r_H = 4.6 → 1.8 au, meaning dust production ∝ r_H^{-1.8±0.3}.	That implies activity driven by a volatile (CO₂ likely).
Tail length / coma size	On ~15 Sept: dust tail ~50 arcseconds ≈ 100,000 km.	Angular size from Earth; depends on geometry.
Gas/volatile production	Mid-Aug 2025: CO₂ gas production ~9.4 × 10¹² molec/s; H₂O upper limit ~1.5 × 10¹² molec/s.	Shows CO₂ dominates over water, unusual for comets.