Light is composed of waves (and particles,. it depends on how you try to measure it). And each color has it’s own respective wave length.
So how can we tell that the universe is expanding? Or if a galaxy is moving toward, or away from us? When the galaxy, as illustrated in the 2nd gif, is moving toward us the light will appear to be blue, (because the blue spectrum of light has a shorter wave length then say the red which is longer). If the galaxy is moving away from us it will appear to be red.
So light can not only reveal things in darkness but tell us how they’re moving through the universe, relative to us. :D Neat!
This liquid is boiling and freezing simultaneously because it’s reaching its ‘triple point,’ which is the temperature and pressure at which three phases of a substance (gas, liquid, and solid) co-exist in equilibrium. Source
Juno captured the thick atmosphere (hydrogen, helium, small amounts of ammonium hydrosulfide) of Jupiter.
Rings upon rings - Messier 95 [4132 x 3956]
Honesty has always a point. [Introductions and footnotes are usually essential though.]
Via
(NASA) The Mysterious Rings of Supernova 1987A Image Credit: ESA/Hubble, NASA
What’s causing those odd rings in supernova 1987A? Twenty five years ago, in 1987, the brightest supernova in recent history was seen in the Large Magellanic Cloud. At the center of the above picture is an object central to the remains of the violent stellar explosion. Surrounding the center are curious outer rings appearing as a flattened figure 8. Although large telescopes including the Hubble Space Telescope monitor the curious rings every few years, their origin remains a mystery. Pictured above is a Hubble image of the SN1987A remnant taken last year. Speculation into the cause of the rings includes beamed jets emanating from an otherwise hidden neutron star left over from the supernova, and the interaction of the wind from the progenitor star with gas released before the explosion.
(NASA) Warped Spiral Galaxy ESO 510-13 Image Credit: Hubble Heritage Team (STScI/AURA), C. Conselice (U. Wisconsin/STScI) et al., NASA
How did spiral galaxy ESO 510-13 get bent out of shape? The disks of many spirals are thin and flat, but not solid. Spiral disks are loose conglomerations of billions of stars and diffuse gas all gravitationally orbiting a galaxy center. A flat disk is thought to be created by sticky collisions of large gas clouds early in the galaxy’s formation. Warped disks are not uncommon, though, and even our own Milky Way Galaxy is thought to have a small warp. The causes of spiral warps are still being investigated, but some warps are thought to result from interactions or even collisions between galaxies. ESO 510-13, pictured above digitally sharpened, is about 150 million light years away and about 100,000 light years across.
Harvard University researchers have developed a new printing method that uses soundwaves to generate droplets from liquids with an unprecedented range of composition and viscosity. This technique could finally enable the manufacturing of many new biopharmaceuticals, cosmetics, and food and expand the possibilities of optical and conductive materials.
“By harnessing acoustic forces, we have created a new technology that enables myriad materials to be printed in a drop-on-demand manner,” said Jennifer Lewis, the Hansjorg Wyss Professor of Biologically Inspired Engineering at the Harvard John A. Paulson School of Engineering and Applied Sciences (SEAS) and the senior author of the paper.
Lewis is also a Core Faculty Member at the Wyss Institute for Biologically Inspired Engineering and the Jianming Yu Professor of Arts and Sciences at Harvard.
The research is published in Science Advances.
Keep reading
Gas pillars inside the Orion Nebula
Here’s a machine that turns water into synthetic gasoline
Lucy Reading-Ikkanda/Quanta Magazine; Source: Feryal Özel