Suspended in a Sunbeam

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Catching Elephant is a theme by Andy Taylor

 

ikenbot: NGC 4038 in Corvus by Hubble Legacy Archive (data); Danny Lee Russell (processing)

ikenbot:

NGC 4038 in Corvus

by Hubble Legacy Archive (data); Danny Lee Russell (processing)

Transit of Saturn by its moons Enceladus, Dione, Titan and Mimas, as seen by Hubble Space Telescope Fun Fact: Saturn has nearly 62 moons with confirmed orbits.  These are the 53 that have been named:Aegaeon Aegir Albiorix Anthe Atlas Bebhionn Bergelmir Bestla Calypso Daphnis Dione Enceladus Epimetheus Erriapus Farbauti Fenrir Fornjot Greip Hati Helene Hyperion Hyrokkin Iapetus Ijiraq Jarnsaxa Janus Kari Kiviuq Loge Methone Mimas Mundilfari Narvi Paaliaq Pallene Pan Pandora Phoebe Polydeuces Prometheus Rhea Suttungr Skathi Siarnaq Skoll Surtur Tarqeq Tarvos Telesto Tethys Thrymr Titan Ymir 

Transit of Saturn by its moons Enceladus, Dione, Titan and Mimas, as seen by Hubble Space Telescope

Fun Fact: Saturn has nearly 62 moons with confirmed orbits. 

These are the 53 that have been named:
Aegaeon 
Aegir 
Albiorix 
Anthe 
Atlas 
Bebhionn 
Bergelmir 
Bestla 
Calypso 
Daphnis 
Dione 
Enceladus 
Epimetheus 
Erriapus 
Farbauti 
Fenrir 
Fornjot 
Greip 
Hati 
Helene 
Hyperion 
Hyrokkin 
Iapetus 
Ijiraq 
Jarnsaxa 
Janus 
Kari 
Kiviuq 
Loge 
Methone 
Mimas 
Mundilfari 
Narvi 
Paaliaq 
Pallene 
Pan 
Pandora 
Phoebe 
Polydeuces 
Prometheus 
Rhea 
Suttungr 
Skathi 
Siarnaq 
Skoll 
Surtur 
Tarqeq 
Tarvos 
Telesto 
Tethys 
Thrymr 
Titan 
Ymir 

Jupiter….my favorite planet since as long as I can remember. And it’s not just because you have the most incredible planet sized moons. 

Jupiter….my favorite planet since as long as I can remember. And it’s not just because you have the most incredible planet sized moons. 

Mariner IV Mars Encounter, circa 1965

Mariner IV Mars Encounter, circa 1965

victorioussleepwalkers: “Look again at that dot. That’s here. That’s home. That’s us. On it everyone you love, everyone you know, everyone you ever heard of, every human being who ever was, lived out their lives. The aggregate of our joy and suffering, thousands of confident religions, ideologies, and economic doctrines, every hunter and forager, every hero and coward, every creator and destroyer of civilization, every king and peasant, every young couple in love, every mother and father, hopeful child, inventor and explorer, every teacher of morals, every corrupt politician, every “superstar”, every “supreme leader”, every saint and sinner in the history of our species lived there—on a mote of dust suspended in a sunbeam.” -Carl Sagan

victorioussleepwalkers:

“Look again at that dot. That’s here. That’s home. That’s us. On it everyone you love, everyone you know, everyone you ever heard of, every human being who ever was, lived out their lives. The aggregate of our joy and suffering, thousands of confident religions, ideologies, and economic doctrines, every hunter and forager, every hero and coward, every creator and destroyer of civilization, every king and peasant, every young couple in love, every mother and father, hopeful child, inventor and explorer, every teacher of morals, every corrupt politician, every “superstar”, every “supreme leader”, every saint and sinner in the history of our species lived there—on a mote of dust suspended in a sunbeam.” -Carl Sagan

Venus, I’ll see you soon. 

Venus, I’ll see you soon. 

scienceblogfortheunwanted:

The first picture (left) was taken by Voyager 2 when it’s path into outer space led it near Neptune. The second one (right) is what Scientists think Neptune is made up of, starting with the outer layer of the atmosphere, and working down into the core.

You can click both pictures for a larger view of them.

ikenbot: How Did Galaxies Form? Image: M81 Spiral galaxy Credit: NASA Spitzer Space Telescope This is one of the questions we still don’t have a conclusive answer to, but as scientists search the cosmos for clues, the mystery becomes clearer. Galaxies probably began to form less than a billion years after the Big Bang, which occurred around 13.7 billion years ago. The primordial Universe consisted almost entirely of hydrogen and helium gas, as well as dark matter, and was, for a time, almost completely homogeneous. It is believed that hypothetical dark matter played a major role in the formation of galaxies and the advent of a heterogeneous Universe. Clouds of gas first began clumping together due to the accumulation of primordial fluctuations, which were small changes of the density in certain parts of the early Universe. Through gravity, gas and dark matter were drawn towards the denser regions of the Universe. There are two main hypotheses on how galaxies began to form, both of which are based on the gravitational effects of collapsing gas. One is called the “bottom-up” theory, in which giant clouds of gas came together in small clumps, which then merged to form larger galaxies. The second theory is the “top-down” one, in which clouds of gas the size of multiple galaxies broke down into individual clumps. This theory would explain why galaxies occur in clusters, and is the most widely accepted model. Hydrogen and helium gas were then drawn towards the inner part of protogalaxies while dark matter formed a halo surrounding the outer part. The gas within these infant galaxies also began to clump together and heat up, forming the first stars. In the beginning, matter in the Universe was composed almost exclusively of hydrogen and helium. Nuclear fusion within stars (and during supernovae) would help make the rest of the heavier elements.

ikenbot:

How Did Galaxies Form?

Image: M81 Spiral galaxy Credit: NASA Spitzer Space Telescope

This is one of the questions we still don’t have a conclusive answer to, but as scientists search the cosmos for clues, the mystery becomes clearer.

Galaxies probably began to form less than a billion years after the Big Bang, which occurred around 13.7 billion years ago. The primordial Universe consisted almost entirely of hydrogen and helium gas, as well as dark matter, and was, for a time, almost completely homogeneous. It is believed that hypothetical dark matter played a major role in the formation of galaxies and the advent of a heterogeneous Universe. Clouds of gas first began clumping together due to the accumulation of primordial fluctuations, which were small changes of the density in certain parts of the early Universe. Through gravity, gas and dark matter were drawn towards the denser regions of the Universe.

There are two main hypotheses on how galaxies began to form, both of which are based on the gravitational effects of collapsing gas. One is called the “bottom-up” theory, in which giant clouds of gas came together in small clumps, which then merged to form larger galaxies. The second theory is the “top-down” one, in which clouds of gas the size of multiple galaxies broke down into individual clumps. This theory would explain why galaxies occur in clusters, and is the most widely accepted model.

Hydrogen and helium gas were then drawn towards the inner part of protogalaxies while dark matter formed a halo surrounding the outer part. The gas within these infant galaxies also began to clump together and heat up, forming the first stars. In the beginning, matter in the Universe was composed almost exclusively of hydrogen and helium. Nuclear fusion within stars (and during supernovae) would help make the rest of the heavier elements.

Planetary Nebula NGC 2438  NGC 2438 is a planetary nebula, the gaseous shroud cast off by a dying sunlike star billions of years old whose central reservoir of hydrogen fuel has been exhausted. About 3,000 light-years distant it lies within the boundaries of the nautical constellation Puppis. Remarkably, NGC 2438 also seems to lie on the outskirts of bright, relatively young open star cluster M46.

Planetary Nebula NGC 2438 

NGC 2438 is a planetary nebula, the gaseous shroud cast off by a dying sunlike star billions of years old whose central reservoir of hydrogen fuel has been exhausted. About 3,000 light-years distant it lies within the boundaries of the nautical constellation Puppis. Remarkably, NGC 2438 also seems to lie on the outskirts of bright, relatively young open star cluster M46.

Orion Nebula & Running Man Nebula.

Orion Nebula & Running Man Nebula.

i-love-fender: Vela Supernova Remnant Credit & Copyright: Robert Gendler Explanation: The plane of our Milky Way Galaxy runs through this complex and beautiful skyscape. At the northwestern edge of the constellation Vela (the Sails) the 16 degree wide, 30 frame mosaic is centered on the glowing filaments of the Vela Supernova Remnant, the expanding debris cloud from the death explosion of a massive star. Light from the supernova explosion that created the Vela remnant reached Earth about 11,000 years ago. In addition to the shocked filaments of glowing gas, the cosmic catastrophe also left behind an incredibly dense, rotating stellar core, the Vela Pulsar. Some 800 light-years distant, the Vela remnant is likely embedded in a larger and older supernova remnant, the Gum Nebula. The broad mosaic includes other identified emission and reflection nebulae, star clusters, and the remarkable Pencil Nebula.

i-love-fender:

Vela Supernova Remnant 
Credit & Copyright: Robert Gendler

Explanation: The plane of our Milky Way Galaxy runs through this complex and beautiful skyscape. At the northwestern edge of the constellation Vela (the Sails) the 16 degree wide, 30 frame mosaic is centered on the glowing filaments of the Vela Supernova Remnant, the expanding debris cloud from the death explosion of a massive star. Light from the supernova explosion that created the Vela remnant reached Earth about 11,000 years ago. In addition to the shocked filaments of glowing gas, the cosmic catastrophe also left behind an incredibly dense, rotating stellar core, the Vela Pulsar. Some 800 light-years distant, the Vela remnant is likely embedded in a larger and older supernova remnant, the Gum Nebula. The broad mosaic includes other identified emission and reflection nebulae, star clusters, and the remarkable Pencil Nebula.

brianyu:

8 Years Around Saturn