NASA released new Artemis lunar flyby images in April 2026—crisp details, deep shadows, and rare angles of the Moon.
Check them out:
Source: Lunar Flyby NASA
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NASA released new Artemis lunar flyby images in April 2026—crisp details, deep shadows, and rare angles of the Moon.
Check them out:
Source: Lunar Flyby NASA
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Artificial intelligence has uncovered a remarkable set of previously unknown cosmic objects hidden within the Hubble Space Telescope’s archival data. Using an AI system developed by the European Space Agency, researchers scanned nearly 100 million image fragments, identifying rare galaxies, gravitational lenses, and other astrophysical anomalies that had gone unnoticed for decades.
This discovery highlights how AI-driven analysis is transforming space imaging and astronomical research. By reanalyzing legacy datasets with modern machine-learning tools, astronomers can rapidly surface new phenomena, unlocking fresh scientific value from historical observations and preparing for the massive data volumes of future space missions.
Source: https://science.nasa.gov/asset/hubble/astrophysical-anomalies-from-hubbles-archive/
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Researchers at the University of Sydney have developed an AI-powered calibration system that restored the James Webb Space Telescope’s interferometric instrument (AMI) without physical intervention.
Their software framework, AMIGO (Aperture Masking Interferometry Generative Observations), employs neural networks and simulation-based modeling to mitigate the brighter-fatter effect, a charge migration phenomenon that caused subtle blurring in JWST images.
The algorithm conducts data-driven deconvolution and point-spread function modeling to reconstruct high-fidelity images, restoring sub-pixel precision and enabling clearer detections of exoplanets, stellar winds, and galactic structures.
This represents a major advance in software-defined optics, demonstrating that mission-critical image correction can be achieved entirely via AI.
Primary Research:
Check out the original post and learn more at ESA’s website.
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On this day, NASA’s STS-31 mission launched the Hubble Space Telescope aboard Space Shuttle Discovery, marking a transformative moment in astronomy.
Since then, Hubble has contributed to over 21,000 peer-reviewed research papers and accumulated more than 1.2 million citations. Its data has significantly advanced our understanding of the cosmos and reinforced the value of space-based telescopes in scientific discovery.
Source: Hubble by the Numbers – NASA
To celebrate its 35th year in orbit, NASA released stunning new images from Hubble.
Check them out: NASA Celebrates Hubble’s 35th Year in Orbit
From swirling galaxies to Martian landscapes, each day brings a new perspective, and honestly, it never gets old.
If you haven’t already, make it part of your daily orbit: https://apod.nasa.gov
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NEO Surveyor is NASA’s upcoming infrared telescope, set to launch in the late 2020s, designed to enhance asteroid detection using heat-based imaging. Unlike Earth-based optical telescopes that rely on visible light, NEO Surveyor detects infrared energy—the heat that asteroids emit. This capability allows it to identify dark or faint space rocks that reflect little light, making it a more effective tool for detecting potential threats that optical telescopes might overlook.
Optical telescopes on Earth struggle to spot asteroids near the Sun because intense sunlight obscures their view. Positioned in space, NEO Surveyor uses infrared technology to cut through this glare, revealing hidden asteroids. Its wide-field camera efficiently scans large portions of the sky, capturing more data in less time compared to ground-based optical systems.
Infrared imaging provides NEO Surveyor with a significant advantage in both clarity and coverage. Unlike optical telescopes, which are affected by Earth’s atmosphere and limited to observing bright objects, this space-based mission offers a clearer, more comprehensive view of near-Earth asteroids. When it comes to tracking space rocks, this advanced technology surpasses traditional methods.
Source: NASA NEO Surveyor Mission
]]>SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer) will use a wide-field spectrophotometer to scan the entire sky in infrared light. This advanced technology will allow scientists to map the cosmic history of galaxies, study water and organic molecules in planetary nurseries, and uncover clues about the universe’s origins.
For more details and to watch the launch, visit NASA’s official page:
SPHEREx Mission Update
Observing distant galaxies is one of the most rewarding experiences for amateur astronomers. However, finding the right telescope can be a challenge, especially when considering factors such as aperture, mount stability, and optical quality. In this article, we explore the best telescope technologies available for amateur astronomers eager to dive into deep-sky observations.
For viewing galaxies, aperture size is crucial because galaxies are often faint objects. Reflector telescopes, particularly Dobsonian models, offer large apertures at an affordable price.
If you prefer automated tracking, GoTo telescopes are ideal. These telescopes feature built-in databases of celestial objects and motorized mounts, making it easy to locate and track galaxies with precision.
For those who want to capture images of galaxies, a combination of a high-quality telescope, a stable equatorial mount, and a sensitive camera is required.
To enhance your galaxy-viewing experience, consider these accessories:
Whether you’re a visual observer or an aspiring astrophotographer, investing in the right telescope technology can make a world of difference in your ability to explore the cosmos. Large-aperture Dobsonians provide the best value for deep-sky observation, while GoTo systems add convenience and ease. If photography is your goal, a high-quality refractor or astrograph on an equatorial mount is the way to go.
Clear skies and happy galaxy hunting!
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