NASA's Parker Solar Probe Hits Record Solar Proximity Amidst Observations of Interstellar Comet 3I/ATLAS
Edited by: Uliana S.
On December 13, 2025, NASA's Parker Solar Probe successfully executed its 26th close approach to the Sun, once again establishing a new record by skimming just 3.8 million miles (6.2 million kilometers) above the star's surface. This maneuver occurred during the peak activity phase of the Sun's 11-year cycle. During this close pass, the spacecraft achieved a blistering top speed of 430,000 miles per hour (687,000 kilometers per hour), setting a new benchmark for speed attained by any human-made object. Mission control, which encompasses the design and assembly of the probe, is managed by the Johns Hopkins University Applied Physics Laboratory (APL) in Maryland. The probe operated autonomously during its closest approach. Communication was fully reestablished with Earth on December 18, 2025, when it transmitted a tone signal confirming that all onboard systems were functioning normally.
The NASA Parker Solar Probe spacecraft captured rare images of the interstellar comet 3I/ATLAS as it passed through the inner Solar System, using its WISPR instrument.
Throughout the period spanning December 8 to December 18, 2025, the probe's four sets of scientific instruments were hard at work, gathering crucial data from directly within the solar corona—the Sun's outermost atmosphere. The information collected during this period of heightened solar activity is absolutely vital for improving forecasts of space weather. Such weather poses tangible risks to satellite infrastructure, astronauts in space, and terrestrial power grids. The Parker Solar Probe mission, which was originally slated for completion, has since been extended. This continuation guarantees that data collection will proceed at least until mid-2029, ensuring further exploration of the extreme conditions characterizing the solar corona.
Running parallel to its primary solar investigation, the Parker Solar Probe also played a role in observing the third confirmed interstellar object, Comet 3I/ATLAS (officially designated C/2025 N1 (ATLAS)). This celestial visitor was first spotted on July 1, 2025, by the ATLAS telescope system located in Chile. It marks only the third known object originating from beyond the boundaries of our Solar System, following in the tracks of 1I/'Oumuamua (spotted in 2017) and 2I/Borisov (spotted in 2019). Comet 3I/ATLAS reached its closest orbital point to the Sun on October 29, 2025.
Between October 18 and November 5, 2025, the WISPR instrument aboard the Parker Solar Probe captured approximately ten images of the comet daily, meticulously documenting its ongoing transformation. Furthermore, NASA's Europa Clipper spacecraft contributed to the study, observing 3I/ATLAS on November 6 from a distance of roughly 102 million miles (164 million kilometers) using its ultraviolet spectrograph. The comet's closest approach to Earth occurred on December 19, 2025, at an approximate distance of 168 million miles (270 million kilometers). The study of 3I/ATLAS sparked considerable scientific discussion, particularly due to observations made by Harvard University astrophysicist Avi Loeb. He highlighted anomalies, such as the presence of a 'counter-tail' and a composition rich in nickel but lacking iron, which naturally led to questions about whether the object was purely cometary. Nevertheless, official statements from NASA representatives have since confirmed that 3I/ATLAS is indeed a comet.
The observations of 3I/ATLAS, which calculations suggest could be up to 7 billion years old and potentially originate from the Milky Way's 'thick disk,' offer an unparalleled chance to examine material formed under conditions vastly different from those in our own stellar neighborhood. The Gemini North telescope also provided supplementary data, revealing shifts in the comet's color profile subsequent to its passage through perihelion. These coordinated observation efforts, involving multiple sophisticated instruments, are yielding a comprehensive analysis of both our home star and these rare visitors from interstellar space.
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