Soon to Pass Earth: Interstellar Comet Captured in New Images

New images show an interstellar comet that will soon make its closest approach to Earth

Astronomers capture new images of interstellar comet 3I/ATLAS approaching Earth

Fresh observations of comet 3I/ATLAS reveal its unusual structure and dynamic tails as it nears its closest approach to Earth later this month. The interstellar visitor, which originated beyond our solar system, has sparked intense interest among scientists since its discovery in July 2025.

Comet 3I/ATLAS represents just the third interstellar object identified as it journeys through our solar system, rendering each observation vital for comprehending its path, makeup, and actions. Detailed images of the comet have been captured by both the Hubble Space Telescope and the European Space Agency’s Jupiter Icy Moons Explorer (Juice) mission, providing unparalleled insight into this extraordinary cosmic event.

Hubble reveals the comet’s teardrop-shaped coma

Hubble first observed 3I/ATLAS shortly after its discovery in July 2025, when the comet was roughly 277 million miles from Earth. Using its Wide Field Camera 3, Hubble documented a distinctive teardrop-shaped halo of dust extending from the comet’s icy nucleus. This glowing cocoon of material highlights the ongoing sublimation of gases and particles as the comet warmed while approaching the sun.

Observations continued on November 30, when the comet was 178 million miles (286 million kilometers) from Earth. Hubble captured even sharper images, allowing astronomers to study the comet’s evolving shape and gas emissions in greater detail. These images are vital for tracking the comet’s path and understanding how interstellar bodies behave when exposed to the sun’s energy.

Juice spacecraft captures dual tails

While Juice’s primary mission is to study Jupiter and its largest moons—Ganymede, Callisto, and Europa, which may host subsurface oceans capable of supporting life—it took advantage of its trajectory to observe comet 3I/ATLAS in early November. From a distance of about 41 million miles (66 million kilometers), the spacecraft used five scientific instruments and its onboard Navigation Camera (NavCam) to record the comet’s activity.

The spacecraft sent a segment of the NavCam data prior to the complete download timeline. The images display a luminous coma surrounding the comet, accompanied by two separate tails: a plasma tail made up of electrically charged gases and a more subtle dust tail composed of solid particles. This dual-tail formation is typical of comets in our solar system; however, witnessing it on an interstellar object offers valuable insights into its physical and chemical characteristics.

Juice’s full dataset, expected to arrive on Earth between February 18 and 20, will include high-resolution images, composition analysis, and particle measurements. These data could shed light on the comet’s origin and the environment it traveled through before entering our solar system.

Close approach to Earth and visibility

Comet 3I/ATLAS is projected to pass within 167 million miles (270 million kilometers) of Earth on December 19, positioning it on the opposite side of the sun and posing no threat to our planet. For context, the Earth orbits roughly 93 million miles (150 million kilometers) from the sun, highlighting that the comet will remain safely distant while still observable by telescopes and space missions.

Even after its closest approach, the comet is expected to remain visible for several months as it continues its journey out of the solar system. Observations during this period will allow scientists to monitor how the comet interacts with solar radiation and the solar wind, further contributing to our understanding of interstellar bodies.

Understanding the Beginnings of Interstellar Phenomena

Studying 3I/ATLAS offers a unique glimpse into material that originated beyond our solar system. The comet’s icy nucleus, surrounded by a cloud of dust and gas, might hold insights into the chemical composition of remote star systems. The tails, influenced by heat and solar radiation, enable scientists to explore how volatile compounds behave when subjected to the sun.

Every interstellar visitor brings unique opportunities to compare our own solar system’s formation with that of other star systems. By analyzing the composition of 3I/ATLAS, scientists hope to uncover information about the types of materials that exist in other parts of the galaxy and how they evolve over time.

Prospects for future studies and research opportunities

The data collected by Hubble and Juice represent only a portion of the potential insights this comet can provide. Upcoming observations from both ground-based and space-based telescopes will help track the comet’s motion, measure its brightness variations, and refine models of its trajectory.

As additional data are received from Juice, scientists expect to gain insights into the dispersion of dust and gas within the coma and tails, the dimensions and spin of the comet’s nucleus, and possible isotopic markers that might unveil the interstellar environment it emerged from. These discoveries could broaden our comprehension of planetary formation, interstellar chemistry, and the frequency of comets moving between star systems.

The unique opportunity presented by 3I/ATLAS underscores the importance of coordinated observations from multiple space missions. By combining high-resolution imaging from Hubble with in-situ measurements from Juice, scientists can create a comprehensive picture of an object that has traveled across the galaxy to reach our solar system.

Comet 3I/ATLAS provides an exceptional view into the vast universe beyond our solar system. Its teardrop-shaped coma, twin tails, and interstellar origins offer invaluable insights for astronomers, while its safe proximity permits ongoing observation from Earth. The continuous analysis of images and data from Hubble and the Juice spacecraft is expected to enhance our comprehension of interstellar objects’ behavior, paving the way for future revelations about the cosmos.

By Mitchell G. Patton

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