Articles

  • 3 weeks ago | wamc.org | Bob Berman

    1 of 1  — strange universe 6-1.png Markus Horn On Sunday night, June 1, enjoy an easy and beautiful sky show: a crescent Moon pairs with two bright stars—one blue-white, one orange. The star just below the Moon is Regulus, the brilliant heart of Leo the Lion, once known as “Qalb” and later named by Copernicus. To the Moon’s right, the orange glow of Mars adds a planetary touch, though it’s dimmer now, sitting on the far side of its orbit.

  • 1 month ago | hudsonvalleyone.com | Bob Berman

    At Memorial Day parties last weekend, I saw many faces I’d known from a half-century ago when I first moved here. All were in their 70’s or beyond. No doubt, some must be contemplating their mortality. So it would seem a good time to offer a very different view of the cosmos, the no-death model, which has a scientific basis despite having not yet generated much awareness.

  • 1 month ago | wamc.org | Bob Berman

    1 of 1  — strange universe 5-25.jpg NASA, ESA, the Hubble Heritage Team (STScI/AURA), A. Nota (ESA/STScI), and the Westerlund 2 Science Team This month look up for a colorful celestial display! Just find the crescent moon in the western sky—sitting in a line with orange-hued Mars and pale blue Regulus, the brightest star in Leo. Together, they create a striking trio of white, orange, and blue—a patriotic parade in the night sky. Tune in to hear when the magic will happen.

  • 1 month ago | wamc.org | Bob Berman

    1 of 1  — STRANGE UNIVERSE.png NASA / iss065e213109 As we enter the moonless phase of the month — ideal for stargazing — it’s worth noting that even the darkest rural skies aren’t truly black. Natural skyglow, made up of airglow, Zodiacal Light, scattered starlight, and the unresolved shimmer of our galaxy, keeps the night subtly illuminated. During this period of solar maximum, the upper atmosphere glows more intensely, making the phenomenon even more striking.

  • 1 month ago | hudsonvalleyone.com | Bob Berman

    That’s a question pondered for centuries: How to permanently leave our world. A cannonball fired upward always returned. With a greater explosive charge and a higher speed, the shell went farther. If aimed sideways, it would start to fall around our planet’s curving surface, extending its travel distance. It wasn’t hard to figure out what speed an object would need to leave permanently. It was 6.9 miles per second. This is Earth’s escape velocity.

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