The Hubble Space Telescope captured this picture of the wispy remains of a supernova explosion. The dust cloud in the upper center of the picture is the actual supernova remnant. The dense concentration of stars in the lower left is the outskirts of star cluster NGC 1850. Full resolution picture here. More info here. Credit: NASA, ESA, Y.-H. Chu (Academia Sinica, Taipei)
Rebel Fleet on approach, weapon systems activated
The Red Rectangle Nebula Image credit: NASA/JPL/ESA
UGC 1810, Wildly Interacting Galaxy from Hubble
Look up and get lost.
Breathtaking views just keep coming! At a distance of 63,400 miles above the cloud tops of Jupiter’s South Pole, the Juno spacecraft reveals incredibly detailed views of the planet’s powerful cyclones and storms.
(Image credit: NASA / MSSS / SwRI / JPL / Caltech. Reprocessing Roman Tkachenko)
The Sun, as of October 8, 2016.
“I’m sorry to disappoint you, but there aren’t any black dwarfs around today. The Universe is simply far too young for it. In fact, the coolest white dwarfs have, to the best of our estimates, lost less than 0.2% of their total heat since the very first ones were created in this Universe. For a white dwarf created at 20,000 K, that means its temperature is still at least 19,960 K, telling us we’ve got a terribly long way to go, if we’re waiting for a true dark star.”
Stars live for a variety of ages, from just a million or two years for some to tens of trillions of years for others. But even after a star has run out of its fuel and died, its stellar corpse continues to shine on. Neutron stars and white dwarfs are both extremely massive, but very small in volume compared to a star. As a result, they cool very slowly, so slow that a single one has not yet gone dark in all the Universe. So how long will it take, and who will get there first: neutron stars or white dwarfs? Believe it or not, there’s still enough uncertainty about how neutron stars cool, mostly due to uncertainties in neutrino physics, that we think we know the answer to be white dwarfs – and 10^14 or 10^15 years – but we’re not entirely sure!
Come find out what we know about finding the first truly dark star in the Universe today.
As Cassini nears the end of its mission, the spacecraft continues to beam back the most astounding images. Last week as it dove between Saturn and its rings, Cassini captured this stunning view of the planet’s beautiful blue vortex. The vortex is an 1,800 mile wide circular storm spinning around Saturn’s pole. Originally captured in black and white, this is the storm in natural color using filters. That vibrant blue is what you’d actually see due to scattering of sunlight, similar Earth’s sky.
(Image credit: NASA/JPL-Caltech/Space Science Institute/Sophia Nasr)