Starry Critters

Tag: pulsar

Fireworks in D

by CritterKeeper on Jun.23, 2010, under Numbers/Letters

Credit: NASA and The Hub­ble Her­itage Team (STScI/AURA)

The let­ter D is out­lined in this celes­tial fire­works dis­play. The col­or­ful fil­a­ments seen in this NASA Hub­ble Space Tele­scope image of N49 are all that’s left of a super­nova explo­sion that took place thou­sands of years ago in the Large Mag­el­lanic Cloud. This super­nova rem­nant is called N 49, or DEM L 190. Inside these sheets of glow­ing star debris lies a pow­er­ful, spin­ning neu­tron star called a pul­sar. Pul­sars give off reg­u­lar pulses of energy like the tick­ing of a very pre­cise clock. After the super­nova blows off the outer lay­ers of the star, it col­lapses under its own grav­ity. The star col­lapses so much that the pro­tons and elec­trons spin­ning around the atoms of the star com­bine to form neu­trons. A neu­tron star is very dense. Imag­ine our entire Sun packed into an area of just 20 kilo­me­ters (12 miles) in diam­e­ter! Grav­ity is very strong on a neu­tron star. On Earth, a spoon­ful of neu­tron star mate­r­ial would weigh bil­lions of tons. The mag­netic field of N 49 is super strong, tril­lions of times stronger than Earth’s, putting it in spe­cial class of bizarre celes­tial objects called magnetars.

(con­tinue read­ing…)

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Monkey Face

by CritterKeeper on Feb.10, 2010, under Bugs, birds and other animals

Credit: NASA and The Hub­ble Her­itage Team (STScI/AURA)

Do you see a mon­key face look­ing up? Or sparks and smoke left over from a fire­works dis­play? The col­or­ful fil­a­ments seen in this NASA Hub­ble Space Tele­scope image of N49 are all that’s left of a super­nova explo­sion that took place thou­sands of years ago in the Large Mag­el­lanic Cloud. This super­nova rem­nant is called N 49, or DEM L 190. Inside these sheets of glow­ing star debris lies a pow­er­ful, spin­ning neu­tron star called a pul­sar. Pul­sars give off reg­u­lar pulses of energy like the tick­ing of a very pre­cise clock. After the super­nova blows off the outer lay­ers of the star, it col­lapses under its own grav­ity. The star col­lapses so much that the pro­tons and elec­trons spin­ning around the atoms of the star com­bine to form neu­trons. A neu­tron star is very dense. Imag­ine our entire Sun packed into an area of just 20 kilo­me­ters (12 miles) in diam­e­ter! Grav­ity is very strong on a neu­tron star. On Earth, a spoon­ful of neu­tron star mate­r­ial would weigh bil­lions of tons. The mag­netic field of N 49 is super strong, tril­lions of times stronger than Earth’s, putting it in spe­cial class of bizarre celes­tial objects called magnetars.

(con­tinue read­ing…)

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The Crab

by CritterKeeper on Aug.25, 2009, under Water Creatures

Credit: NASA, ESA, J. Hes­ter and A. Loll (Ari­zona State University)

In the year 1054, Japan­ese, Chi­nese and Native Amer­i­can astronomers recorded a vio­lent event. They saw a star that hadn’t been there before. It turned out to be a super­nova that formed the Crab Neb­ula and it’s one of the ear­li­est recorded astro­nom­i­cal events by humans.

(con­tinue read­ing…)

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