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NASA Astronomy Picture of the Day:

What’s creating this giant hole in space? This is not a black hole — it’s a shadow. It’s Earth’s shadow. Since at least the time of Aristotle, people have noted that Earth's dark shadow on the Moon during a partial lunar eclipse is circular -- although never a whole circle. Using modern digital technology, though, the images of multiple lunar eclipses can be combined to show Earth's complete shadow. The featured image compilation by a perseistent astrophotographer is constructed from 22 years of lunar eclipses. The Moon is not eclipsed every month (moon-th) because the Moon's orbit is slightly tilted relative to Earth's orbit. Close inspection of some lunar eclipse images shows a faint blue band where Earth’s atmosphere filters out more red sunlight than blue. Later this week, a new lunar eclipse will occur and will be best visible in parts of North and South America, Europe, and Africa. APOD's main NASA site is moving : From apod.nasa.gov to science.nasa.gov/apod

Photo by Tim Martin

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Comet 220P in Outburst

Posted by Specola- • Profile • 08/24/26 at 02:16PM • Science and Technology • See more by Specola-

NASA Astronomy Picture of the Day:

Comet 220P is unexpectedly bright. Normally, periodic Comet 220P/McNaught is so dim that to see it requires a telescope. Two surprising outbursts this year, however, have made it about 20,000 times brighter than usual, so that it is now visible with binoculars and long-duration camera exposures. As expected, Comet 220P continues to orbit the Sun between Mars and Jupiter with a period of over 5 years. The featured long duration exposure, taken 10 days ago from South Africa, shows the comet's bright green head and short dust tail. Reasons for Comet 220P's impressive outbursts are unknown but could be caused by the release of built-up subsurface gas or comet quakes. Comet 220P will pass about one Earth-Sun distance from the Earth in October, after which it is expected to fade quickly as it begins its return to the far part of its orbit. APOD's main NASA site is moving : From apod.nasa.gov to science.nasa.gov/apod

Photo by Spilios Asimakopoulos

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Musings, Quotes & Proverbs CONTRIBUTOR

Clive Staples Lewis (1898 - 1963) C. S. Lewis was a British novelist, poet, academic, literary critic, essayist, lay theologian, broadcaster and lecturer. 

Science and Technology Series CONTRIBUTOR

NASA Astronomy Picture of the Day:

What would it look like to approach the grand planet Saturn? One doesn't have to just imagine -- the Cassini spacecraft did just this in 2004, recording thousands of images along the way, and hundreds of thousands more since entering orbit. Some of Cassini's early images have been digitally tweaked, cropped, and compiled into the featured inspiring video which is part of a larger IMAX movie project named In Saturn's Rings. In the concluding sequence, Saturn looms increasingly large on approach as cloudy Titan swoops below. With Saturn whirling around in the background, Cassini is next depicted flying over Mimas, with large Herschel Crater clearly visible. Saturn's majestic rings then take over the show as Cassini crosses Saturn's thin ring plane. Dark shadows of the ring appear on Saturn itself. Finally, the enigmatic ice-geyser moon Enceladus appears in the distance and then is approached just as the video clip ends. After more than a decade of exploration and discovery, the Cassini spacecraft ran low on fuel in 2017 was directed to enter Saturn's atmosphere, where it surely melted. APOD's main NASA site is moving : From apod.nasa.gov to science.nasa.gov/apod

Video by Cassini Imaging Team, ISS, JPL, NASA, ESA, S. Van Vuuren et al.; Music: Adagio for Strings (NY Philharmonic)

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The Joy of Walking Without a Destination | Kudos365 Life Series

In a world that often measures success by how quickly we reach the next destination, there is something refreshing about taking a walk with nowhere in particular to go. Without a schedule to keep or an errand to complete, walking becomes less about arriving and more about noticing. It offers an opportunity to slow our pace, observe our surroundings, and enjoy the simple experience of being present.

Science and Technology Series CONTRIBUTOR

NASA Astronomy Picture of the Day:

Recorded the night of August 12-13, images from four dedicated meteor-monitoring cameras at an astronomical observatory in Czechia were aligned and combined to create this all-night, all-sky view. On that night, the total count came to 1,706 meteors. And since that coincided with the peak activity of the 2026 Perseid Meteor Shower, most are perseids. Their overwhelming numbers make them easy to spot. Quite convincingly, perseid trails all trace back to a single radiant on the sky at the upper right, a region in the annual shower's eponymous constellation Perseus. But meteors belonging to other much less active showers can also revealed by finding their radiants too. For example, seen crossing the perseid trails are meteors from a shower whose radiant lies in Cygnus, known as Kappa Cygnids. The antihelion complex, a general region near Aquarius and opposite the Sun in the sky, is also identifiable as a weak source for meteors.

Photo by Valašské Meziříčí Observatory

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History Series CONTRIBUTOR

History Challenge || August 22, 2026

Posted by Kronos • Profile • 08/22/26 at 12:00AM • History • See more by Kronos

Welcome to Kudos365 Weekly History Challenge. Test your history  knowledge and see how many of the history questions you can answer correctly. A new updated History Challenge is released every Saturday.

Science and Technology Series CONTRIBUTOR

NASA Astronomy Picture of the Day:

What does it feel like to zoom around a spinning supermassive black hole? The featured video is an animation showing a time-lapse of 4 years of observations of the star S301 orbiting Sagittarius A*, the 4-million-solar-mass black hole in the center of our Galaxy. S301 was discovered in 2023 with the Very Large Telescope Interferometer of the European Southern Observatory, located in the Atacama Desert in Chile. Astronomers recently found that S301 takes approximately 8.7 years to go around the black hole and reaches speeds of 25,000 km/s. It comes closer to the black hole than any other stars detected before, at a distance similar to that from Saturn to the Sun. Because it comes so close to Sagittarius A*, S301 could be used to directly measure how fast the black hole spins and test Einstein's theory of general relativity. According to the theory, a spinning black hole drags the fabric of spacetime around itself, affecting the orbits of close-by objects.

Watch NASA's Astronomy Video of the Day

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