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Nice. Now all we need is to get solar panels everywhere.
Nice. Now all we need is to get solar panels everywhere.
Lol. You can never have too much space.We're gonna need a biggerboatgalaxy.
Speaking of space being big…Lol. You can never have too much space.
Too bad I'll never get to see it.
If you're in or near the US northeast... there's a Solar System in Maine! :nerdy:Too bad I'll never get to see it.
If you're in or near the US northeast... there's a Solar System in Maine! :nerdy:
Really interesting. And all of that just for the nearest star system - all of which is an invisible speck for the size of the universe.Speaking of space being big…
You can get “scale models” of the Solar System. However, such models are only to scale with respect to the relative sizes of the Sun and planets. Size and distance would be quite impossible to depict with a desktop toy. But online, there are DIY instructions on how to build a true scale model. One is called the “peppercorn Solar System” (best constructed in a large field ).
The Sun is represented by a soccer ball (or large cantaloupe); and Mercury (the first planet) is the head of a pin. So much for size. For distance, you’d need to pace out 10 yards (!) to get the proper scale of Mercury’s orbit. (At this scale, the soccer ball is still easy enough to see. But good luck trying to spot the pinhead.) Next, you pace out an additional 9 yards from pinhead/Mercury (19 yards from the soccer ball/Sun) to get to Venus — represented by a peppercorn. Then, an additional 7 yards (26 yards total) will get you to Earth — also a peppercorn.
From there, the distances only get bigger. By the time you place the model of Neptune at its proper relative distance, you’ll have walked 777 yards (!). (Indeed, you might need a pair of binoculars to see back to your soccer ball/Sun.) And keep in mind, these distances only represent the radius of the Solar System model. The diameter would be twice this size.
If you’re feeling ambitious, you might try setting up a model of the nearest star system: the Alpha Centauri system. But at the “peppercorn scale,” the Alpha Centauri A soccer ball would need to be about 4000 miles away...
So, yeah. There’s a lot of space in space.
Saturn's Northern Hexagon
Image Credit & Copyright: NASA, ESA, JPL, SSI, Cassini Imaging Team
Explanation: Why would clouds form a hexagon on Saturn? Nobody is sure. Originally discovered during the Voyager flybys of Saturn in the 1980s, nobody has ever seen anything like it anywhere else in the Solar System. Acquiring its first sunlit views of far northern Saturn in late 2012, the Cassini spacecraft's wide-angle camera recorded this stunning, false-color image of the ringed planet's north pole. The composite of near-infrared image data results in red hues for low clouds and green for high ones, giving the Saturnian cloudscape a vivid appearance. This and similar images show the stability of the hexagon even 20+ years after Voyager. Movies of Saturn's North Pole show the cloud structure maintaining its hexagonal structure while rotating. Unlike individual clouds appearing like a hexagon on Earth, the Saturn cloud pattern appears to have six well defined sides of nearly equal length. Four Earths could fit inside the hexagon. Beyond the cloud tops at the upper right, arcs of the planet's eye-catching rings are tinted bright blue.
Lol, those crazy aliens. They'll do anything to impress.Some aliens saw Pentagon and decided to make something more impressive.
“The expected signal is the random ‘background’ ocean of these gravitational waves, which is the sum of the waves from every binary supermassive black hole in the universe,” said Daniel Reardon, an astronomer at Swinburne University of Technology and a member of OzGrav, in an email to Gizmodo. “Observing this gravitational-wave background has important consequences for our understanding of the formation history of our universe, because supermassive black holes are the engines at the heart of galaxies.”
Gravitational waves were first predicted by Einstein in his theory of general relativity. As described by Einstein, the waves are changes to a gravitational field that travel at the speed of light. Indeed, gravitational waves emerge from seismic interactions of the universe’s most massive and compact objects. When black holes orbit or collide with each other, or other very dense objects like neutron stars, gravitational waves are produced by the interaction.
Nice to see things we only guessed at finally being proven. Yay, science!Gizmodo - Wild Webb image uncovers carbon molecule in distant star system.
A carbon-based ion—likely an important building block of interstellar carbon chemistry—was spotted in a protoplanetary disk 1,350 light-years away.
Scientific American - In a First, Scientists See Neutrinos Emitted by the Milky Way
The disk of our galaxy was long thought to produce these ghostly high-energy particles, but they haven’t been detected until now