Equatorial Diameter: 51.118 km
Satellites: 27
Notable satellites: Oberon, Titania, Miranda, Ariel & Umbriel
Orbit Distance: 2.870.658.186 km (19 AU)
Orbit Period: 84 Earth years
Surface Temperature: -220°C
Discovered Date: March 13th 1781
Discovered By: William Herschel
Image credit: Oscar Malet
Sequence of images of auroras seen at the south pole of Saturn. Images combine visible and ultraviolet light.
Credit: NASA, ESA, J. Clarke (Boston University, USA), and Z. Levay (STScI)
Meteor impact craters of the world
Image of Titan taken by the Cassini spacecraft
NASA/JPL-Caltech/SSI/Kevin M. Gill
Remnant of supernova toward the constellation of Vela, which exploded 11,000 years ago.
Image credit: NASA / Chandra x-ray Observatory
This new NASA/ESA Hubble Space Telescope image shows the center of the Lagoon Nebula, an object with a deceptively tranquil name, in the constellation of Sagittarius. The region is filled with intense winds from hot stars, churning funnels of gas, and energetic star formation, all embedded within an intricate haze of gas and pitch-dark dust.
Image Credit: NASA/JPL/ESA/J. Trauger
A slow-motion animation of the Crab Pulsar taken at 800 nm wavelength (near-infrared) using a Lucky Imaging camera from Cambridge University, showing the bright pulse and fainter interpulse.
Credit: Cambridge University Lucky Imaging Group
Low genetic diversity is a problem when you’re founding a new colony, so how would we avoid that on another planet?
This image shows an artist’s impression of the 10 Hot Jupiter Exoplanets studied using the Hubble and Spitzer Space Telescopes. From the upper left to the lower right corner, these planets are WASP-12b, WASP-6b, WASP-31b, WASP-39b, HD 189733b, HAT-P-12b, WASP-17b, WASP-19b, HAT-P-1b And HD 209458b.
Credit: ESA / Hubble & NASA
Pulsars are spherical, compact objects that are about the size of a large city but contain more mass than the sun. Discovered in 1967, pulsars are fascinating members of the cosmic community.
From Earth, pulsars often look like flickering stars. On and off, on and off, they seem to blink with a regular rhythm. But the light from pulsars does not actually flicker or pulse, and these objects are not actually stars.
Pulsars radiate two steady, narrow beams of light in opposite directions. Although the light from the beam is steady, pulsars appear to flicker because they also spin. It’s the same reason a lighthouse appears to blink when seen by a sailor on the ocean: As the pulsar rotates, the beam of light may sweep across the Earth, then swing out of view, then swing back around again. To an astronomer on the ground, the light goes in and out of view, giving the impression that the pulsar is blinking on and off. The reason a pulsar’s light beam spins around like a lighthouse beam is that the pulsar’s beam of light is typically not aligned with the pulsar’s axis of rotation.
Click here to see the animation
Click here to hear the pulsars sound
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