Starship Asterisk*

[quote="neufer"][quote="orin stepanek"]

Is it possible that the SMC & the LMC at one time was (were) one galaxy and that the Milky Way ripped it apart? :?[/quote]
If so you would have to explain why the two have distinctive chemical compositions:
[quote=" http://asterisk.apod.com/viewtopic.php?f=31&t=31905&p=204994#p204994"]

<<[Andrew J. Fox]'s team found a low amount of oxygen and sulfur along most of the stream, matching the levels in the Small Magellanic Cloud about 2 billion years ago, when the gaseous ribbon was thought to have been formed.

In a surprising twist, the team discovered a much higher level of sulfur in a region closer to the Magellanic Clouds. "We're finding a consistent amount of heavy elements in the stream until we get very close to the Magellanic Clouds, and then the heavy element levels go up," said Fox. "This inner region is very similar in composition to the Large Magellanic Cloud, suggesting it was ripped out of that galaxy more recently.">>[/quote][/quote]

So the SMC is more metallic than the LMC? Would that make the stars in the SMC younger, on average, and of latter generations than those of the LMC? That would lead to the conclusion that the SMC has the greater possibility of terrestrial planets, teeny tiny rocks with carbon and real "metal" metals. Which would make it the better candidate for aliens.

APoD is so cool. It's like a random dip into a vast ocean of knowledge and mystery every day.

Something I tried to do but don't have the software to manage, could this Stream image be converted into a rotatable sphere? That would be neat.

So much going on we don't really see.....

:---[===] *

"sitelines"? Sightlines?

[quote="orin stepanek"]

Is it possible that the SMC & the LMC at one time was (were) one galaxy and that the Milky Way ripped it apart? :?[/quote]
If so you would have to explain why the two have distinctive chemical compositions:
[quote=" http://asterisk.apod.com/viewtopic.php?f=31&t=31905&p=204994#p204994"]

<<[Andrew J. Fox]'s team found a low amount of oxygen and sulfur along most of the stream, matching the levels in the Small Magellanic Cloud about 2 billion years ago, when the gaseous ribbon was thought to have been formed.

In a surprising twist, the team discovered a much higher level of sulfur in a region closer to the Magellanic Clouds. "We're finding a consistent amount of heavy elements in the stream until we get very close to the Magellanic Clouds, and then the heavy element levels go up," said Fox. "This inner region is very similar in composition to the Large Magellanic Cloud, suggesting it was ripped out of that galaxy more recently.">>[/quote]

Is it possible that the SMC & the LMC at one time was (were) one galaxy and that the Milky Way ripped it apart? :?

Somehow, today's APOD reminds me splattered-paint abstract art.

Could probably print and sell it for millions! :mrgreen:

Now they found the heart of our milkyway :- http://earthsky.org/science-wire/a-magnetar-at-the-heart-of-our-milky-way

Just to let you know, the "Tomorrow's APOD" link from yesterday doesn't work. Fortunately there are alternate routes to get here from there.

Nice video, Beyond! :D

Yes, the Large Magellanic Cloud is stealing matter from the Small Magellanic Cloud, and both clouds are losing matter in the process. Where does this missing matter go? Some is just "lost in space", I'm sure. But quite a lot of it may end up in the Mikly Way, replenishing our galaxy with gas and dust and fuelling star formation.

Ann

Yesterday, this APOD was billed as Islands in the Stream. So i went out and found a song to fit. As it turns out, i found it in the Large MGM cloud of people.

[youtube]http://www.youtube.com/watch?v=2nvR_7mJtMk[/youtube]

[url=http://apod.nasa.gov/apod/ap130815.html][img]http://apod.nasa.gov/apod/calendar/S_130815.jpg[/img] [size=150]The Magellanic Stream[/size][/url]

[b] Explanation: [/b] [url=http://hubblesite.org/newscenter/archive/releases/2013/27/]In an astronomical version[/url] of the search for the source [url=http://www.historytoday.com/richard-cavendish/nile%E2%80%99s-source-discovered]of the Nile[/url], astronomers now have strong evidence for the origin of the [url=http://astronomy.swin.edu.au/cosmos/M/Magellanic+Stream]Magellanic Stream[/url]. This composite image shows the long ribbon of gas, discovered at radio wavelengths in the 1970s, in pinkish hues against an optical all-sky view across the plane of our Milky Way galaxy. Both Large and Small [url=http://apod.nasa.gov/apod/ap060809.html]Magellanic Clouds[/url], dwarf satellite galaxies of the the Milky Way, are seen near the head of the stream at the right. Data from Hubble's [url=http://hubblesite.org/the_telescope/nuts_.and._bolts/instruments/cos/]Cosmic Origins Spectrograph[/url] were used to [url=http://arxiv.org/abs/1304.4240]explore abundances[/url] of elements along sitelines to quasars that intersect the stream. The results indicate that most of the stream's material comes from the Small Magellanic Cloud. The Magellanic Stream is likely the result of gravitational tidal interactions [url=http://arxiv.org/abs/1008.2210]between the two dwarf galaxies[/url] some 2 billion years ago, the Small Magellanic Cloud losing more material in the encounter because of its lower mass.

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