JWST Discovery Today - James Webb Telescope Uncovers Atmosphere on Sizzling Lava Planet TOI-561 b
Stunning Hubble Space Telescope image of interstellar comet 3I/ATLAS captured on November 30, 2025, showing its glowing light blue coma and central nucleus amid streaked stars. As this third known interstellar visitor nears its December 19, 2025, Earth approach, Hubble reveals its ethereal beauty. Credit: NASA, ESA, STScI, D. Jewitt (UCLA)
Updated on December 15, 2025 | By Jameswebb Discovery Editorial Team
A comet potentially older than the Sun, ejected from a distant star system billions of years ago, is currently racing through the solar system. On December 19, 2025, interstellar comet 3I/ATLAS will reach its closest approach to Earth at approximately 1.8 AU (around 167 million miles). This rare event offers a unique opportunity to study an object from beyond the solar system.Officially designated C/2025 N1 (ATLAS), 3I/ATLAS stands as the third confirmed interstellar object detected. Its hyperbolic trajectory confirms it is merely passing through, unbound by the Sun's gravity. Observations from the James Webb Space Telescope (JWST) have revealed an unusual CO2-dominated composition, while recent images display an expanding tail and indications of cryovolcanic activity. Search terms such as "3I/ATLAS facts," "interstellar comet 3I/ATLAS closest approach," and "JWST 3I/ATLAS observations" lead to this comprehensive resource, featuring the latest December 2025 updates and visuals.
Discovered on July 1, 2025, by the NASA-funded ATLAS telescope in Chile.
Initially tagged as A11pl3Z, later officially named C/2025 N1 (ATLAS).
The "3I" prefix identifies it as the third interstellar object, after 1I/'Oumuamua and 2I/Borisov.
Appeared faint at magnitude 18 upon discovery, requiring large telescopes for visibility.
Precovery images from NASA's TESS satellite extend back to May 2025.
Interstellar status confirmed on July 2, 2025, based on its extreme orbit.
Initially mistaken by some for a rocky asteroid until coma development was observed.
Rapid follow-up observations came from teams at over 30 observatories worldwide.
The announcement of hyperbolic eccentricity confirmed another genuine interstellar traveler.
The ATLAS survey, focused on near-Earth threats, achieved this significant detection.
Eccentricity approximately 6.14, far exceeding 1 and proving unbound status.
Incoming speed around 58 km/s, among the highest recorded.
Perihelion on October 29, 2025, at 1.36 AU.
Maximum speed exceeded 68 km/s near the Sun.
Inclination near 175 degrees, retrograde yet aligned close to the ecliptic plane.
Closest Earth approach on December 19, 2025, at 1.798 AU—completely safe.
Passed Mars at 0.19 AU in October 2025.
Approaches Venus in November 2025 and Jupiter in March 2026.
Origin from the galactic thick disk, opposite typical stellar motion directions.
Age estimates range from 3 to 14 billion years—truly ancient.
Outgassing provides minor non-gravitational acceleration.
Current position on December 15, 2025: Visible in Leo during pre-dawn hours.
Brightness near magnitude 11—accessible with small telescopes under dark skies.
Brightness increasing slightly as Earth aligns post-perihelion.
Minimum distance nearly twice the Earth-Sun separation, posing no risk.
Path crosses constellations from Sagittarius through Virgo to Leo.
Opposition in January 2026 offers extended viewing, though fading occurs rapidly.
Obscured by solar conjunction in October; now fully observable.
Dynamical models indicate past stellar encounters influenced its trajectory.
Such orbits provide insights into ejection processes in other star systems.
Eccentricity: 6.14 (unbound; bound comets below 1)
Perihelion: 1.36 AU
Inclination: 175° (retrograde and unusual)
Earth Closest: 1.798 AU on Dec 19, 2025
Excess Speed: 58 km/s (extremely high)
Nucleus size estimated between 0.5 and 5.6 km (Hubble upper limit).
Mass comparable to a small mountain.
Rotation period around 16 hours.
Reddish coloration similar to distant Kuiper Belt objects.
Extensive coma reaching hundreds of thousands of km, dominated by CO2.
JWST August observations: CO2-to-water ratio approximately 8—highly anomalous.
Detected gases include CO2, water ice, CO, and rare carbonyl sulfide.
Low water content suggests formation distant from its parent star.
Isotopic analysis indicates low-metallicity origin system.
Ground-based detections of cyanide and nickel, with depletion in certain carbon compounds.
Activity initiated beyond 6 AU, driven by CO2 sublimation.
Recent indications point to cryovolcanic eruptions.
Sunward jets and anti-tail currently visible.
Dust tail extending significantly post-perihelion.
Polarization consistent with pristine ancient material.
Fine amorphous water ice grains detected far from nucleus.
Steady activity observed without major outbursts.
Brightness peaked near magnitude 11, stable during close approach.
Asymmetric coma with fan-shaped dust features.
Composition differs markedly from solar system comets, impacting planet formation models.
JWST August 6 data highlighted prominent CO2 plume.
Additional JWST sessions scheduled for December 2025 to monitor outbound evolution.
Hubble captured images in July and November to constrain nucleus size.
Ultraviolet spectroscopy tracking gas emissions.
Combined with SPHEREx for water ice confirmation.
JWST infrared capabilities excel at detecting distant ices.
Possible thick crust concealing deeper water reserves.
Formation likely beyond CO snow line in original system.
Publications in ApJ Letters describe findings as transformative.
Spectra offer glimpses into extrasolar chemical processes.
Observations from Hubble, JWST, and spacecraft including JUICE and Psyche.
Gemini telescopes produced detailed color composites.
Very Large Telescope detected CN and nickel emissions.
Swift telescope identified early water signatures.
Amateur images now capture anti-tail transitioning to full tail.
XMM-Newton examined X-ray interactions with solar wind.
Activity remains steady without fragmentation.
Mars orbiters recorded the close Mars passage.
Archives contain hundreds of observations.
Marginal visibility possible in binoculars under ideal conditions.
Probable ejection via giant planet or stellar encounter billions of years ago.
Thick disk origin implies older, metal-poor environment.
Speculation regarding artificial nature exists, though consensus confirms natural cometary origin.
Speed precludes any interception mission.
Indicates abundant interstellar objects throughout the galaxy.
Demonstrates wide variation in extrasolar chemistries.
Cryovolcanism provides clues to internal structure.
Activity exhibits heartbeat-like patterns.
Significant implications for exoplanet formation theories.
Serves as a reminder of galactic wanderers.
Speed establishes new cometary records.
Red hue aligns with primitive solar system bodies.
Dust production rates increasing currently.
Potential heavy isotopes from early stellar generations.
Challenges traditional water-driven activity models.
Resembles trans-Neptunian objects more than typical comets.
Tail now detectable in small telescopes.
Optimal pre-dawn views in Leo approaching soon.
Fading rapidly after January, departing permanently.
JWST prepared for future interstellar detections.
Exemplifies outstanding global scientific collaboration.
Amateur astronomers contribute valuable data.
Safe passage yet timed thrillingly.
CO2 dominance stands out as a key surprise.
Connects solar system studies to exoplanets.
Acts as a time capsule from Milky Way history.
Visibility peaks near closest approach.
Sightings welcomed in comments for community sharing.
This rare event should not be missed.
Clear skies—3I/ATLAS represents a once-in-a-generation visitor.
Interstellar comet 3I/ATLAS stands apart from the only two prior confirmed interstellar objects—1I/'Oumuamua (2017) and 2I/Borisov (2019)—in several key ways that highlight the diversity of extrasolar bodies. Its record-breaking hyperbolic excess velocity of approximately 58 km/s surpasses both predecessors ('Oumuamua at 26 km/s and Borisov at 32 km/s), indicating a longer journey through interstellar space and potentially an ancient origin in the Milky Way's thick disk, with age estimates reaching 7–14 billion years. JWST observations reveal an unusually CO2-dominated coma (CO2-to-water ratio around 8), contrasting sharply with Borisov's carbon monoxide richness and 'Oumuamua's lack of detectable activity or coma. Additional distinctions include a larger estimated nucleus (up to 5.6 km), reddish dust similar to D-type asteroids yet with unique depletions in carbon chains, and early activation driven by CO2 sublimation far from the Sun. These features make 3I/ATLAS a vital bridge for understanding varied planetary formation processes across the galaxy, challenging models derived from solar system comets and underscoring why searches for "interstellar comet 3I/ATLAS unique features" and "3I/ATLAS vs Oumuamua Borisov" continue to draw attention ahead of its December 19, 2025, Earth approach.
This interstellar comet provides pristine material from another stellar system, illuminated through JWST and Hubble observations. During its December 19 approach, pre-dawn views in Leo are recommended with a telescope. Safe, stunning, and transient, it offers a fleeting glimpse into the cosmos.
ESA/NASA SOHO mission observation of interstellar comet 3I/ATLAS from October 15-26, 2025, capturing the faint brightening in the center during its perihelion passage behind the Sun. This rare coronagraph view highlights the comet's activity as it rounded the Sun before emerging for Earth-based viewing ahead of its December 19, 2025, closest approach. Credit: Lowell Observatory/Qicheng Zhang