Moon and Griffith Observatory

View larger. | Full moon and Griffith Observatory in Los Angeles. Photo by Josh Blash. See more of Josh's photography on Facebook.

View larger. | Bright moon from Griffith Observatory, November 27, 2015. Photo by Josh Blash. See more of Josh’s photography on Facebook.

Our friend Josh Blash submitted this photo to EarthSky this weekend. It’s Friday night’s moon, next to the famous Griffith Observatory in Los Angeles. This observatory is know for its public viewing nights and other activities. Josh wrote:

Hello Earthsky!

While waiting in line to use the telescope Friday night, I caught this picture of the moon behind the Zeiss telescope dome at the Griffith Observatory. It was crowded but it was nice to see so many people taking an interest in the cosmos!

Canon 6D 35mm

Thank you, Josh!



from EarthSky http://ift.tt/1XoOtdG
View larger. | Full moon and Griffith Observatory in Los Angeles. Photo by Josh Blash. See more of Josh's photography on Facebook.

View larger. | Bright moon from Griffith Observatory, November 27, 2015. Photo by Josh Blash. See more of Josh’s photography on Facebook.

Our friend Josh Blash submitted this photo to EarthSky this weekend. It’s Friday night’s moon, next to the famous Griffith Observatory in Los Angeles. This observatory is know for its public viewing nights and other activities. Josh wrote:

Hello Earthsky!

While waiting in line to use the telescope Friday night, I caught this picture of the moon behind the Zeiss telescope dome at the Griffith Observatory. It was crowded but it was nice to see so many people taking an interest in the cosmos!

Canon 6D 35mm

Thank you, Josh!



from EarthSky http://ift.tt/1XoOtdG

Old broken links [Stoat]

At some point SB moved wordpress versions, and when this occurred old links broke. Every now and again when I come across an old post I fix them up, but you can’t, so here is the sekret decoder ring. Things like:

http://ift.tt/1Ren5tZ

turn into

http://ift.tt/1OJ3OgA

Which is annoying, because whilst you can get from “new” to “old” by s/-/_/g, removing the extra number and adding “.php”, you can’t get from old to new without knowing the number. Argh! But, it turns out the server has been taught some intelligence, because

http://ift.tt/1Ren5u1

does work; it redirects to “new”. Don’t forget s/_/-/g.



from ScienceBlogs http://ift.tt/1MMBJ8B

At some point SB moved wordpress versions, and when this occurred old links broke. Every now and again when I come across an old post I fix them up, but you can’t, so here is the sekret decoder ring. Things like:

http://ift.tt/1Ren5tZ

turn into

http://ift.tt/1OJ3OgA

Which is annoying, because whilst you can get from “new” to “old” by s/-/_/g, removing the extra number and adding “.php”, you can’t get from old to new without knowing the number. Argh! But, it turns out the server has been taught some intelligence, because

http://ift.tt/1Ren5u1

does work; it redirects to “new”. Don’t forget s/_/-/g.



from ScienceBlogs http://ift.tt/1MMBJ8B

Can we see stars outside our Milky Way?

Photo at top of post by Jeff Dai in Tibet. Read more about this image.

One of you wrote:

Are there any stars outside our own galaxy that we can see with just the eye?

The answer is no – unless you count seeing the combined light of many billions of stars. From the Northern Hemisphere, the only galaxy outside our Milky Way that’s easily visible to the eye is the great galaxy in the constellation Andromeda, also known as M31. More about the Andromeda galaxy at the bottom of this post.

From the Southern Hemisphere, it’s possible to see two dwarf galaxies, the Large and Small Magellanic Clouds.

So what are we seeing when we look up? The image at the top of this post shows a hazy band in the sky. This is the edgewise view into our own Milky Way galaxy. Our galaxy is about 100,000 light-years in a diameter, but it’s relatively flat, only about 10,000 light-years thick. So – if we’re looking in a dark sky – when we look toward the galactic disk, we see the starry band of the Milky Way.

And when we look up or down – away from the flat disk of the galaxy – we’re also seeing Milky Way stars. All of the stars we see with the eye alone belong to our Milky Way galaxy.

EarthSky astronomy kits are perfect for beginners. Order today from the EarthSky store

View larger. Anthony Lynch Photography provided this beauty of a Perseid meteor and the Andromeda galaxy. Thank you Anthony!

View larger. Anthony Lynch Photography provided this beauty of photo in August, 2015. It’s a colorful Perseid meteor and the Andromeda galaxy. Thank you Anthony!

It is possible to see the Andromeda galaxy with the eye alone, from Earth’s Northern Hemisphere. This galaxy appears as a hazy patch in our night sky, about as wide in diameter as a full moon. And, indeed, this haze represents the light of the Andromeda galaxy’s billions of stars. But we still can’t see individual stars within this galaxy – not with the eye alone. Even with amateur telescopes, the patch of light that we see as the Andromeda galaxy looks, at best, like haze.

Earlier this year, astronomers released a new sharpest-ever view of the Andromeda galaxy.

And you can see the galaxy for yourself. In late November, the Andromeda galaxy is visible from nightfall till about 4 a.m. Here are a couple of ways to find the galaxy:

Use Great Square of Pegasus to find Andromeda galaxy

Or …

Use constellation Cassiopeia to find Andromeda galaxy

Be sure to look for it in a dark sky, far from city lights. Good luck!

Bottom line: On a dark night, there are so many stars. Are any of the stars we see with the eye alone located beyond our home galaxy? The answer is no. All the stars we see with the eye alone belong to our Milky Way. But there is one distant galaxy you can see from

Astronomy events, star parties, festivals, workshops for September-December, 2015

Almost gone! EarthSky lunar calendars make great gifts. Order now.

Donate: Your support means the world to us



from EarthSky http://ift.tt/1NgjeGF

Photo at top of post by Jeff Dai in Tibet. Read more about this image.

One of you wrote:

Are there any stars outside our own galaxy that we can see with just the eye?

The answer is no – unless you count seeing the combined light of many billions of stars. From the Northern Hemisphere, the only galaxy outside our Milky Way that’s easily visible to the eye is the great galaxy in the constellation Andromeda, also known as M31. More about the Andromeda galaxy at the bottom of this post.

From the Southern Hemisphere, it’s possible to see two dwarf galaxies, the Large and Small Magellanic Clouds.

So what are we seeing when we look up? The image at the top of this post shows a hazy band in the sky. This is the edgewise view into our own Milky Way galaxy. Our galaxy is about 100,000 light-years in a diameter, but it’s relatively flat, only about 10,000 light-years thick. So – if we’re looking in a dark sky – when we look toward the galactic disk, we see the starry band of the Milky Way.

And when we look up or down – away from the flat disk of the galaxy – we’re also seeing Milky Way stars. All of the stars we see with the eye alone belong to our Milky Way galaxy.

EarthSky astronomy kits are perfect for beginners. Order today from the EarthSky store

View larger. Anthony Lynch Photography provided this beauty of a Perseid meteor and the Andromeda galaxy. Thank you Anthony!

View larger. Anthony Lynch Photography provided this beauty of photo in August, 2015. It’s a colorful Perseid meteor and the Andromeda galaxy. Thank you Anthony!

It is possible to see the Andromeda galaxy with the eye alone, from Earth’s Northern Hemisphere. This galaxy appears as a hazy patch in our night sky, about as wide in diameter as a full moon. And, indeed, this haze represents the light of the Andromeda galaxy’s billions of stars. But we still can’t see individual stars within this galaxy – not with the eye alone. Even with amateur telescopes, the patch of light that we see as the Andromeda galaxy looks, at best, like haze.

Earlier this year, astronomers released a new sharpest-ever view of the Andromeda galaxy.

And you can see the galaxy for yourself. In late November, the Andromeda galaxy is visible from nightfall till about 4 a.m. Here are a couple of ways to find the galaxy:

Use Great Square of Pegasus to find Andromeda galaxy

Or …

Use constellation Cassiopeia to find Andromeda galaxy

Be sure to look for it in a dark sky, far from city lights. Good luck!

Bottom line: On a dark night, there are so many stars. Are any of the stars we see with the eye alone located beyond our home galaxy? The answer is no. All the stars we see with the eye alone belong to our Milky Way. But there is one distant galaxy you can see from

Astronomy events, star parties, festivals, workshops for September-December, 2015

Almost gone! EarthSky lunar calendars make great gifts. Order now.

Donate: Your support means the world to us



from EarthSky http://ift.tt/1NgjeGF

The UK should not bomb Syria [Stoat]

In fact I’m not quite as certain of the Right Thing as my headline suggests; but if I’m going to nail my colours to the mast in advance of the UK’s parliament’s probable vote next week, I may as well be definite. It puts me with Jeremy Corbyn and against most of the UK pols. I don’t feel involved enough to go and protest, though, as I did before the Iraq war. More that two years ago I wrote words that could be interpreted as support for military intervention. But that was more than two years ago; things have changed since. Most of what has changed has changed for the worse; the country is more broken; the chances of tilting the balance in favour of the Good Guys by bombing is pretty well gone.

The govt’s reasons for action are available. It is a long document; although page 11 onwards is “Response to Questions in the Foreign Affairs Committee report on “Enabling the House to reach a decision” ” and is effectively an appendix; but much of page 1 is blather, and page 2 begins That is why I believe that we should now take the decision to extend British airstrikes against ISIL [in Iraq] into Syria, so we deduce that there’s one key paragraph on page 1 to read. It is:

We need a comprehensive response which seeks to deal with the threat that ISIL poses to us directly, not just through the measures we are taking at home, but by dealing with ISIL on the ground in the territory that it controls. It is in Raqqa, Syria, that ISIL has its headquarters, and it is from Raqqa that some of the main threats against this country are planned and orchestrated. We must tackle ISIL in Syria, as we are doing in neighbouring Iraq, in order to deal with the threat that ISIL poses to the region and to our security here at home. We have to deny a safe haven for ISIL in Syria. The longer ISIL is allowed to grow in Syria, the greater the threat it will pose. It is wrong for the United Kingdom to sub-contract its security to other countries, and to expect the aircrews of other nations to carry the burdens and the risks of striking ISIL in Syria to stop terrorism here in Britain.

That contains a number of arguments not clearly separated; probably because they’re weaker when clearly and distinctly made.

1. Increase the UK’s security. Arguably a somewhat selfish attitude, but also part of the government’s core responsibility. But the applicability of this argument seems implausible to me; indeed, the reverse seems more likely to be true. The govt’s doc has a longer section on “The Threat from ISIL”, with stuff like We know that ISIL has deadly intent to strike us at home too. In the last 12 months, Britain’s police and Security Services have disrupted no fewer than 7 terrorist plots to attack the UK. All 7 plots were either linked to ISIL, or were inspired by ISIL’s propaganda. Whether you find that “undeniable” evidence of a threat to the UK is perhaps a matter of judgement; mine is that it doesn’t, and that I don’t trust the govt’s judgement.

2. “It is wrong for the United Kingdom to sub-contract its security to other countries” is a two-part argument. The first is the “altruistic” quasi-moral part: we shouldn’t let other people do our fighting for us. And this is true, if we believe the fighting is a good idea; but it doesn’t help decide if said fighting is good. The contrary – we shouldn’t bother, since our military contribution is small and neither here-nor-there – isn’t very believable either; its along the same lines as those who argue that we shouldn’t trouble about our CO2 emissions, because on a global scale they are small. The second, implicit, part is that we shouldn’t undermine other’s efforts by hanging back. But again, that doesn’t help you decide of the efforts are good.

3. What we’re doing in Iraq argues that we should do the same in Syria. But there’s a key difference: in Iraq, we’re acting on behalf of and with the cooperation of an at least nominally friendly government. It seems to be that concentrating any military efforts there would be more fruitful. The previous, notoriously sectarian and incompetent Iraq government, bears a large share of the responsibility for the rise of ISIS; if it hadn’t let so much of Iraq get taken over, ISIS wouldn’t have got its early boost (note: I’m willing to be corrected on the details of that). But we-the-West also bear our share, for propping up such a disastrous government. Having done my best to consider this carefully, it seems likely that the most useful route to removing ISIS begins by fixing Iraq’s government. That’s a long term process, liable to be tedious and difficult, and involve things like supporting and enhancing democracy. And in the short term, doing our little bit to help the US support the Iraqi’s astonishingly incompetent army. The govt says By inflicting brutal attacks against his own people, Assad has in fact acted as one of ISIL’s greatest recruiting sergeants. We therefore need a political transition in Syria to a government that the international community can work with against ISIL, as we already do with the Government of Iraq. However, I can’t see any signs of such a transition actually happening, so that crucial part of the govt’s strategy is broken.

4. “The longer ISIL is allowed to grow in Syria, the greater the threat it will pose”. This is almost believeable. It might be true; or it might not – since any concentration of ISIS is vulnerable to air attack, its hard for them to grow such concentrations.

Arguments against bombing include “the Iraq war was a disaster”. And indeed it was; and you can make a decent case that disaster has lead directly to this one, albeit with many other mistakes along the way. But that argument is something of a logical fallacy, in the way its usually presented; somewhat along the lines of “but you were all predicting an ice age in the 1970’s”. In another way, in that the same kind of people who made the same kind of mistakes will be in charge again, its not a fallacy.

The recent attacks on France are why the French are so hot and why we may get involved; effectively, something so close to home provides motivation. What prevents similar here? Mostly, I’d guess, the difficulty of getting hold of Kalashnikovs. We’re probably not short of nutters; but the nutters are (thankfully) short of guns. This strongly suggests to me that doing more to get rid of the guns would be a good idea. While we’re here, I’ll note that the total death toll on French roads in 2013 was 3250; not-at-all-to-anyone’s-surprise, this hasn’t provoked horror or outrage.

Another argument against bombing might be the cost, if only I knew what it was. This piece says that 7 months in Libya (which I supported) cost ~$380 million; perhaps for the purposes of discussion I could guess that Syria would cost the UK £500 million a year. That’s not large enough to be a convincing argument against (but for comparison, we say we’ve donated £1.1 billion “providing assistance to ease the suffering of the Syrian people”). But I argue that the bomb money would be better spent on helping Syrian refugees in Turkey, and similar matters; not just in terms of bread-not-bombs being better for the world, but in terms of security.

Another item is that govt’s, and the press, and the public, can only focus on a few things at once, with enough pressure to get things done. Pushing so hard on bomb-Syria means other things can’t be pushed.

Not having Russia in Syria deliberately targetting non-ISIS opponents of Assad would help a lot; but I can’t see any way to avoid their presence; Russia as elsewhere is just being malignant.

I don’t like the govt’s degrade and ultimately defeat ISIL, including through Coalition military and wider action because I’m suspicious of the “degrade”. It is such a vague term; used by the US too; it amounts to “well, yes, we blew some things up and killed some bad guys but really we don’t have much of a plan beyond that”.

What would you do, then?

The obvious question, which I’ve partially answered above: help in Iraq, and provide aid. Another element, which I’ve referred to before, would be to end our obsession with border lines drawn on maps many years ago; and to support a Kurdish state.

Another possible question is “what would the people inside Syria like us to do?” I find I have no idea at all what the answer is.



from ScienceBlogs http://ift.tt/1NicVH6

In fact I’m not quite as certain of the Right Thing as my headline suggests; but if I’m going to nail my colours to the mast in advance of the UK’s parliament’s probable vote next week, I may as well be definite. It puts me with Jeremy Corbyn and against most of the UK pols. I don’t feel involved enough to go and protest, though, as I did before the Iraq war. More that two years ago I wrote words that could be interpreted as support for military intervention. But that was more than two years ago; things have changed since. Most of what has changed has changed for the worse; the country is more broken; the chances of tilting the balance in favour of the Good Guys by bombing is pretty well gone.

The govt’s reasons for action are available. It is a long document; although page 11 onwards is “Response to Questions in the Foreign Affairs Committee report on “Enabling the House to reach a decision” ” and is effectively an appendix; but much of page 1 is blather, and page 2 begins That is why I believe that we should now take the decision to extend British airstrikes against ISIL [in Iraq] into Syria, so we deduce that there’s one key paragraph on page 1 to read. It is:

We need a comprehensive response which seeks to deal with the threat that ISIL poses to us directly, not just through the measures we are taking at home, but by dealing with ISIL on the ground in the territory that it controls. It is in Raqqa, Syria, that ISIL has its headquarters, and it is from Raqqa that some of the main threats against this country are planned and orchestrated. We must tackle ISIL in Syria, as we are doing in neighbouring Iraq, in order to deal with the threat that ISIL poses to the region and to our security here at home. We have to deny a safe haven for ISIL in Syria. The longer ISIL is allowed to grow in Syria, the greater the threat it will pose. It is wrong for the United Kingdom to sub-contract its security to other countries, and to expect the aircrews of other nations to carry the burdens and the risks of striking ISIL in Syria to stop terrorism here in Britain.

That contains a number of arguments not clearly separated; probably because they’re weaker when clearly and distinctly made.

1. Increase the UK’s security. Arguably a somewhat selfish attitude, but also part of the government’s core responsibility. But the applicability of this argument seems implausible to me; indeed, the reverse seems more likely to be true. The govt’s doc has a longer section on “The Threat from ISIL”, with stuff like We know that ISIL has deadly intent to strike us at home too. In the last 12 months, Britain’s police and Security Services have disrupted no fewer than 7 terrorist plots to attack the UK. All 7 plots were either linked to ISIL, or were inspired by ISIL’s propaganda. Whether you find that “undeniable” evidence of a threat to the UK is perhaps a matter of judgement; mine is that it doesn’t, and that I don’t trust the govt’s judgement.

2. “It is wrong for the United Kingdom to sub-contract its security to other countries” is a two-part argument. The first is the “altruistic” quasi-moral part: we shouldn’t let other people do our fighting for us. And this is true, if we believe the fighting is a good idea; but it doesn’t help decide if said fighting is good. The contrary – we shouldn’t bother, since our military contribution is small and neither here-nor-there – isn’t very believable either; its along the same lines as those who argue that we shouldn’t trouble about our CO2 emissions, because on a global scale they are small. The second, implicit, part is that we shouldn’t undermine other’s efforts by hanging back. But again, that doesn’t help you decide of the efforts are good.

3. What we’re doing in Iraq argues that we should do the same in Syria. But there’s a key difference: in Iraq, we’re acting on behalf of and with the cooperation of an at least nominally friendly government. It seems to be that concentrating any military efforts there would be more fruitful. The previous, notoriously sectarian and incompetent Iraq government, bears a large share of the responsibility for the rise of ISIS; if it hadn’t let so much of Iraq get taken over, ISIS wouldn’t have got its early boost (note: I’m willing to be corrected on the details of that). But we-the-West also bear our share, for propping up such a disastrous government. Having done my best to consider this carefully, it seems likely that the most useful route to removing ISIS begins by fixing Iraq’s government. That’s a long term process, liable to be tedious and difficult, and involve things like supporting and enhancing democracy. And in the short term, doing our little bit to help the US support the Iraqi’s astonishingly incompetent army. The govt says By inflicting brutal attacks against his own people, Assad has in fact acted as one of ISIL’s greatest recruiting sergeants. We therefore need a political transition in Syria to a government that the international community can work with against ISIL, as we already do with the Government of Iraq. However, I can’t see any signs of such a transition actually happening, so that crucial part of the govt’s strategy is broken.

4. “The longer ISIL is allowed to grow in Syria, the greater the threat it will pose”. This is almost believeable. It might be true; or it might not – since any concentration of ISIS is vulnerable to air attack, its hard for them to grow such concentrations.

Arguments against bombing include “the Iraq war was a disaster”. And indeed it was; and you can make a decent case that disaster has lead directly to this one, albeit with many other mistakes along the way. But that argument is something of a logical fallacy, in the way its usually presented; somewhat along the lines of “but you were all predicting an ice age in the 1970’s”. In another way, in that the same kind of people who made the same kind of mistakes will be in charge again, its not a fallacy.

The recent attacks on France are why the French are so hot and why we may get involved; effectively, something so close to home provides motivation. What prevents similar here? Mostly, I’d guess, the difficulty of getting hold of Kalashnikovs. We’re probably not short of nutters; but the nutters are (thankfully) short of guns. This strongly suggests to me that doing more to get rid of the guns would be a good idea. While we’re here, I’ll note that the total death toll on French roads in 2013 was 3250; not-at-all-to-anyone’s-surprise, this hasn’t provoked horror or outrage.

Another argument against bombing might be the cost, if only I knew what it was. This piece says that 7 months in Libya (which I supported) cost ~$380 million; perhaps for the purposes of discussion I could guess that Syria would cost the UK £500 million a year. That’s not large enough to be a convincing argument against (but for comparison, we say we’ve donated £1.1 billion “providing assistance to ease the suffering of the Syrian people”). But I argue that the bomb money would be better spent on helping Syrian refugees in Turkey, and similar matters; not just in terms of bread-not-bombs being better for the world, but in terms of security.

Another item is that govt’s, and the press, and the public, can only focus on a few things at once, with enough pressure to get things done. Pushing so hard on bomb-Syria means other things can’t be pushed.

Not having Russia in Syria deliberately targetting non-ISIS opponents of Assad would help a lot; but I can’t see any way to avoid their presence; Russia as elsewhere is just being malignant.

I don’t like the govt’s degrade and ultimately defeat ISIL, including through Coalition military and wider action because I’m suspicious of the “degrade”. It is such a vague term; used by the US too; it amounts to “well, yes, we blew some things up and killed some bad guys but really we don’t have much of a plan beyond that”.

What would you do, then?

The obvious question, which I’ve partially answered above: help in Iraq, and provide aid. Another element, which I’ve referred to before, would be to end our obsession with border lines drawn on maps many years ago; and to support a Kurdish state.

Another possible question is “what would the people inside Syria like us to do?” I find I have no idea at all what the answer is.



from ScienceBlogs http://ift.tt/1NicVH6

Comments of the Week #87: From Quasars to Einstein, and Thanksgiving [Starts With A Bang]

“At times our own light goes out and is rekindled by a spark from another person. Each of us has cause to think with deep gratitude of those who have lighted the flame within us.” -Albert Schweitzer

It was an action-packed week here at Starts With A Bang, where we took on all of the following:

 

There’s so much more that’s on its way, including our second podcast coming next week, an upcoming holiday giveaway for the lucky submissions chosen for Ask Ethan, and some more spectacular articles about how the Universe came to be, and how we know it. (Oh, and we’ve also almost unlocked the next Patreon reward, for real! Let’s make it happen before 2015 is out!)

Now, join me as we jump in to our Comments of the Week!

Image credit: ISS astronaut Scott Kelly, via https://twitter.com/StationCDRKelly/status/666042034633883649/photo/1?ref_src=twsrc%5Etfw.

Image credit: ISS astronaut Scott Kelly, via https://twitter.com/StationCDRKelly/status/666042034633883649/photo/1?ref_src=twsrc%5Etfw.

From Dean on the “UFO” seen from the ISS: “‘As I explain, however, this is simply light reflecting off of the ISS’s HDEV module, nothing more complex or extraordinary than that.’
That’s what they WANT us to believe. :)

What’s kind of remarkable is that no one caught my real mistake: it wasn’t the HDEV module at all that caused the reflection, but rather the window shutter to the ESA’s Destiny’s Lab.

Image credit: ISS / NASA, with annotations by Sam Treadgold.

Image credit: ISS / NASA, with annotations by Sam Treadgold.

So, I suppose, it could be construed as a case of Europeans pranking Americans, and our tendencies to “want to believe.” This is what we get for having American Thanksgiving, isn’t it, Europe?

Image credit: NASA/JPL-Caltech.

Image credit: NASA/JPL-Caltech.

From Gary S on dark matter hairs vs. haze: “Is there some reason to think the (undetectable!) dark matter particles have a [preferred] travel direction near our solar system? If not, then there would be no “hairs” – just a haze around massive bodies with only slightly increased concentration.”

There are two things that I want to respond to here, one of which you’ve realized and one that you haven’t. Dark matter particles are expected to move in a virialized fashion, which means their velocities should be randomly distributed with a gradient towards/away from the center of gravity. The Earth’s motion — around the Sun and through the galaxy — should be added/subtracted from that.

In addition, we don’t think that dark matter should have the same rotational speed around the center that the normal matter does, so Earth should be moving, on average at 190-250 km/s relative to the dark matter.

Image credit: Gary Prezeau, via http://ift.tt/1Io51Fb.

Image credit: Gary Prezeau, via http://ift.tt/1Io51Fb.

But then there’s this part: the focusing part. If there’s dark matter coming in at the same trajectory, which there ought to be, the planet’s gravity will focus that into a stream, and then into a hair. Commenter Wow made an allusion to this when he said:

“Gary, the idea is that this is a similar thing to [gravitational] lensing, where gravity makes a stream of particles bend their path, refracting to a focal point.”

The main difference is that there is a velocity dispersion and an impact parameter range here, which leads to the development of a hair. The important point, though, is that this fluffy, diffuse “cloud” of dark matter will generically give rise to a caustic, or a point where the density spikes incredibly high, the same way that a magnifying glass focuses the Sun’s rays to a point.

Image credit: flickr user Dave Gough, via http://ift.tt/1uIy9A8.

Image credit: flickr user Dave Gough, via http://ift.tt/1uIy9A8.

This is a generic behavior of cold, collisionless dark matter, even if it’s isothermally distributed. This was shown by Pierre Sikivie in (I believe) 1995, and is accepted and used by astrophysicists everywhere. It’s even referenced in Gary Prezeau’s paper. Sikivie was on my thesis defense committee; it’s amazing how small the world of cosmology truly is.

Image credit: The Observatories of the Carnegie Institution for Science Collection at the Huntington Library, San Marino, Calif.

Image credit: The Observatories of the Carnegie Institution for Science Collection at the Huntington Library, San Marino, Calif.

From Gary S on the successor to the Hooker 100″ telescope: ““Mt. Wilson, which then housed a telescope twice as large…”
If you meant the 200 inch, isn’t that on Mt. Palomar?”

The 200″ Hale was on Mt. Palomar instead of Mt. Wilson, you are correct. The 100″ was on Mt. Wilson and Hubble was the primary name associated with both. What’s interesting is the 100″, commissioned in 1917, was the largest in the world until the Hale, with only Otto Struve’s 82″ telescope (in the 1930s) coming close. When the 200″ was commissioned in the late 1940s, it was the largest until the Soviet BTA-6 in 1976 and the second largest until the Keck telescope in the 1990s.

Image credit: Wikimedia Commons user Cmglee.

Image credit: Wikimedia Commons user Cmglee.

What I think is remarkable is the advent of segmented mirrors and of telescope arrays. No longer are we limited by what glass can do under the force of gravity, but rather by finances alone. More area = more light = more power, and when it comes to exploring the distant Universe, that means more details, more data, and more knowledge.

Image credit: NASA / JPL.

Image credit: NASA / JPL.

From Hephaestus on comets and Oort clouds: “People always refer to passing stars disturbing our Oort cloud and launching a comet Sun-ward. What about the Sun disturbing other stars’ clouds and drawing off one or more of their Oortlets? We must be near the edge of the Centauri system’s cloud.”

Don’t let a diagram like this — which is on a logarithmic scale — fool you. The Oort cloud may go out as far as about half a light year, but the gravitational binding is extraordinarily tenuous. When a star comes close by us, which happens every few 100,000 years or so, our Oort cloud objects get perturbed, and so do theirs.

Image credit: Michael Osadciw/University of Rochester.

Image credit: Michael Osadciw/University of Rochester.

Yes, these stars should have their own Oort clouds, and the mutual interactions should perturb both our Oort cloud objects and also theirs. But consider the difference between these two scenarios:

  1. 50% of our perturbed Oort cloud objects will lose velocity with respect to our Sun, reducing their orbits and sending them closer to the inner Solar System. A few of these — the ones that lose the most heliocentric velocity — get close enough to the Sun to become comets.
  2. 50% of the other star’s perturbed Oort cloud objects will gain velocity with respect to its Sun, many (perhaps most) of which will be ejected from their solar system. But only a tiny percentage will wind up being directed towards our inner Solar System, and an even smaller fraction will get an additional gravitational interaction that causes them to wind up on a stable (elliptical, rather than hyperbolic) orbit.

So it’s possible, but we can say with 98%+ certainty that each comet we see from the Oort cloud is from our Oort cloud.

Image credit: Keck / UCLA galactic center group / A. Ghez et al., via http://ift.tt/1XyIA8C.

Image credit: Keck / UCLA galactic center group / A. Ghez et al., via http://ift.tt/1XyIA8C.

From Waterbergs on a black hole’s event horizon: “Does this mean the event horizon of the [black holes] gets squashed out of spherical into some increasingly strange shape? As I understand it [Sagittarius] A* has a mass of about 4 million solar masses. If one assumes each [black] hole contributed around 20 solar masses then this means 200 000 black holes merged to create it.”

The event horizon of a non-rotating black hole is spherical; the event horizon of a rotating black hole is not. What’s really fun here is that the singularity of a non-rotating black hole is a point; the event horizon of a rotating black hole is a ring, or a 1-dimensional singularity rather than a 0-dimensional one.

It isn’t the act of mergers that cause the distortion; it’s the end state, and how much angular momentum it has. The event horizon winds up being ellipsoidal rather than spherical, and more technically like an oblate spheroid. Fun, but counterintuitive stuff!

Image credit: Wikimedia Commons user Brews ohare.

Image credit: Wikimedia Commons user Brews ohare.

And finally, from Denier as a follow-up on the Lemaître/Hubble controversy: “When originally learning of this story, I seem to remember the reason the critical portion wasn’t translated was because Albert Einstein criticized it. Prior to publication, he shared his finding with Einstein who replied with something to the affect of ‘I can’t find any fault in your math but your physics are atrocious’. Lemaître held Einstein in high esteem, and that scorching rebuke caused Lemaître to doubt his own work. The section wasn’t translated because Lemaître was trying to save himself from further ridicule.”

Einstein said a lot of dismissive, wrongheaded things, particularly after 1915. He derided every new development in quantum physics; he railed against the developing science of particle physics; he constantly returned to his old, discredited ideas; he failed to appreciate the nuance and insight of his contemporaries like Pauli, Schrodinger, Bohr, Dirac and others. In short, Einstein got left behind.

This is very different than my favorite stories from the book Denier refers to: The Very First Light by Mather and Boslough, which really give some insight into how dogmatic Fred Hoyle was. He was so repulsed by the idea that the Big Bang could be right, because it seemed to jive somewhat with a biblical story and because the innovation could be connected to Lemaître, a priest, that he never let a shred of evidence sway his opinion. In short, despite all the developments he initiated in stellar nucleosynthesis and other areas of cosmology and astrophysics, he became one of the saddest stories in all of late 20th century science.

Image credit: E. Siegel and World Scientific.

Image credit: E. Siegel and World Scientific.

Those of you who want to learn more about that particular time of development in science will particularly enjoy chapters 4-6 of my book, Beyond The Galaxy: how humanity looked beyond the Milky Way and discovered the entire Universe. It’s available for your holiday shopping now, for pre-order and for 30% off with the code WS15XMAS30 at checkout. Get copies for yourself, and for all your science-minded friends, today!



from ScienceBlogs http://ift.tt/1XyIAp1

“At times our own light goes out and is rekindled by a spark from another person. Each of us has cause to think with deep gratitude of those who have lighted the flame within us.” -Albert Schweitzer

It was an action-packed week here at Starts With A Bang, where we took on all of the following:

 

There’s so much more that’s on its way, including our second podcast coming next week, an upcoming holiday giveaway for the lucky submissions chosen for Ask Ethan, and some more spectacular articles about how the Universe came to be, and how we know it. (Oh, and we’ve also almost unlocked the next Patreon reward, for real! Let’s make it happen before 2015 is out!)

Now, join me as we jump in to our Comments of the Week!

Image credit: ISS astronaut Scott Kelly, via https://twitter.com/StationCDRKelly/status/666042034633883649/photo/1?ref_src=twsrc%5Etfw.

Image credit: ISS astronaut Scott Kelly, via https://twitter.com/StationCDRKelly/status/666042034633883649/photo/1?ref_src=twsrc%5Etfw.

From Dean on the “UFO” seen from the ISS: “‘As I explain, however, this is simply light reflecting off of the ISS’s HDEV module, nothing more complex or extraordinary than that.’
That’s what they WANT us to believe. :)

What’s kind of remarkable is that no one caught my real mistake: it wasn’t the HDEV module at all that caused the reflection, but rather the window shutter to the ESA’s Destiny’s Lab.

Image credit: ISS / NASA, with annotations by Sam Treadgold.

Image credit: ISS / NASA, with annotations by Sam Treadgold.

So, I suppose, it could be construed as a case of Europeans pranking Americans, and our tendencies to “want to believe.” This is what we get for having American Thanksgiving, isn’t it, Europe?

Image credit: NASA/JPL-Caltech.

Image credit: NASA/JPL-Caltech.

From Gary S on dark matter hairs vs. haze: “Is there some reason to think the (undetectable!) dark matter particles have a [preferred] travel direction near our solar system? If not, then there would be no “hairs” – just a haze around massive bodies with only slightly increased concentration.”

There are two things that I want to respond to here, one of which you’ve realized and one that you haven’t. Dark matter particles are expected to move in a virialized fashion, which means their velocities should be randomly distributed with a gradient towards/away from the center of gravity. The Earth’s motion — around the Sun and through the galaxy — should be added/subtracted from that.

In addition, we don’t think that dark matter should have the same rotational speed around the center that the normal matter does, so Earth should be moving, on average at 190-250 km/s relative to the dark matter.

Image credit: Gary Prezeau, via http://ift.tt/1Io51Fb.

Image credit: Gary Prezeau, via http://ift.tt/1Io51Fb.

But then there’s this part: the focusing part. If there’s dark matter coming in at the same trajectory, which there ought to be, the planet’s gravity will focus that into a stream, and then into a hair. Commenter Wow made an allusion to this when he said:

“Gary, the idea is that this is a similar thing to [gravitational] lensing, where gravity makes a stream of particles bend their path, refracting to a focal point.”

The main difference is that there is a velocity dispersion and an impact parameter range here, which leads to the development of a hair. The important point, though, is that this fluffy, diffuse “cloud” of dark matter will generically give rise to a caustic, or a point where the density spikes incredibly high, the same way that a magnifying glass focuses the Sun’s rays to a point.

Image credit: flickr user Dave Gough, via http://ift.tt/1uIy9A8.

Image credit: flickr user Dave Gough, via http://ift.tt/1uIy9A8.

This is a generic behavior of cold, collisionless dark matter, even if it’s isothermally distributed. This was shown by Pierre Sikivie in (I believe) 1995, and is accepted and used by astrophysicists everywhere. It’s even referenced in Gary Prezeau’s paper. Sikivie was on my thesis defense committee; it’s amazing how small the world of cosmology truly is.

Image credit: The Observatories of the Carnegie Institution for Science Collection at the Huntington Library, San Marino, Calif.

Image credit: The Observatories of the Carnegie Institution for Science Collection at the Huntington Library, San Marino, Calif.

From Gary S on the successor to the Hooker 100″ telescope: ““Mt. Wilson, which then housed a telescope twice as large…”
If you meant the 200 inch, isn’t that on Mt. Palomar?”

The 200″ Hale was on Mt. Palomar instead of Mt. Wilson, you are correct. The 100″ was on Mt. Wilson and Hubble was the primary name associated with both. What’s interesting is the 100″, commissioned in 1917, was the largest in the world until the Hale, with only Otto Struve’s 82″ telescope (in the 1930s) coming close. When the 200″ was commissioned in the late 1940s, it was the largest until the Soviet BTA-6 in 1976 and the second largest until the Keck telescope in the 1990s.

Image credit: Wikimedia Commons user Cmglee.

Image credit: Wikimedia Commons user Cmglee.

What I think is remarkable is the advent of segmented mirrors and of telescope arrays. No longer are we limited by what glass can do under the force of gravity, but rather by finances alone. More area = more light = more power, and when it comes to exploring the distant Universe, that means more details, more data, and more knowledge.

Image credit: NASA / JPL.

Image credit: NASA / JPL.

From Hephaestus on comets and Oort clouds: “People always refer to passing stars disturbing our Oort cloud and launching a comet Sun-ward. What about the Sun disturbing other stars’ clouds and drawing off one or more of their Oortlets? We must be near the edge of the Centauri system’s cloud.”

Don’t let a diagram like this — which is on a logarithmic scale — fool you. The Oort cloud may go out as far as about half a light year, but the gravitational binding is extraordinarily tenuous. When a star comes close by us, which happens every few 100,000 years or so, our Oort cloud objects get perturbed, and so do theirs.

Image credit: Michael Osadciw/University of Rochester.

Image credit: Michael Osadciw/University of Rochester.

Yes, these stars should have their own Oort clouds, and the mutual interactions should perturb both our Oort cloud objects and also theirs. But consider the difference between these two scenarios:

  1. 50% of our perturbed Oort cloud objects will lose velocity with respect to our Sun, reducing their orbits and sending them closer to the inner Solar System. A few of these — the ones that lose the most heliocentric velocity — get close enough to the Sun to become comets.
  2. 50% of the other star’s perturbed Oort cloud objects will gain velocity with respect to its Sun, many (perhaps most) of which will be ejected from their solar system. But only a tiny percentage will wind up being directed towards our inner Solar System, and an even smaller fraction will get an additional gravitational interaction that causes them to wind up on a stable (elliptical, rather than hyperbolic) orbit.

So it’s possible, but we can say with 98%+ certainty that each comet we see from the Oort cloud is from our Oort cloud.

Image credit: Keck / UCLA galactic center group / A. Ghez et al., via http://ift.tt/1XyIA8C.

Image credit: Keck / UCLA galactic center group / A. Ghez et al., via http://ift.tt/1XyIA8C.

From Waterbergs on a black hole’s event horizon: “Does this mean the event horizon of the [black holes] gets squashed out of spherical into some increasingly strange shape? As I understand it [Sagittarius] A* has a mass of about 4 million solar masses. If one assumes each [black] hole contributed around 20 solar masses then this means 200 000 black holes merged to create it.”

The event horizon of a non-rotating black hole is spherical; the event horizon of a rotating black hole is not. What’s really fun here is that the singularity of a non-rotating black hole is a point; the event horizon of a rotating black hole is a ring, or a 1-dimensional singularity rather than a 0-dimensional one.

It isn’t the act of mergers that cause the distortion; it’s the end state, and how much angular momentum it has. The event horizon winds up being ellipsoidal rather than spherical, and more technically like an oblate spheroid. Fun, but counterintuitive stuff!

Image credit: Wikimedia Commons user Brews ohare.

Image credit: Wikimedia Commons user Brews ohare.

And finally, from Denier as a follow-up on the Lemaître/Hubble controversy: “When originally learning of this story, I seem to remember the reason the critical portion wasn’t translated was because Albert Einstein criticized it. Prior to publication, he shared his finding with Einstein who replied with something to the affect of ‘I can’t find any fault in your math but your physics are atrocious’. Lemaître held Einstein in high esteem, and that scorching rebuke caused Lemaître to doubt his own work. The section wasn’t translated because Lemaître was trying to save himself from further ridicule.”

Einstein said a lot of dismissive, wrongheaded things, particularly after 1915. He derided every new development in quantum physics; he railed against the developing science of particle physics; he constantly returned to his old, discredited ideas; he failed to appreciate the nuance and insight of his contemporaries like Pauli, Schrodinger, Bohr, Dirac and others. In short, Einstein got left behind.

This is very different than my favorite stories from the book Denier refers to: The Very First Light by Mather and Boslough, which really give some insight into how dogmatic Fred Hoyle was. He was so repulsed by the idea that the Big Bang could be right, because it seemed to jive somewhat with a biblical story and because the innovation could be connected to Lemaître, a priest, that he never let a shred of evidence sway his opinion. In short, despite all the developments he initiated in stellar nucleosynthesis and other areas of cosmology and astrophysics, he became one of the saddest stories in all of late 20th century science.

Image credit: E. Siegel and World Scientific.

Image credit: E. Siegel and World Scientific.

Those of you who want to learn more about that particular time of development in science will particularly enjoy chapters 4-6 of my book, Beyond The Galaxy: how humanity looked beyond the Milky Way and discovered the entire Universe. It’s available for your holiday shopping now, for pre-order and for 30% off with the code WS15XMAS30 at checkout. Get copies for yourself, and for all your science-minded friends, today!



from ScienceBlogs http://ift.tt/1XyIAp1

2015 SkS Weekly News Roundup #48

A chronological listing of the news articles posted on the Skeptical Science Facebook page during the past week.

Sun, Nov 22

Mon, Nov 23

Tue, Nov 24

Wed, Nov 25

Thu, Nov 26

Fri, Nov 27

Sat, Nov 28



from Skeptical Science http://ift.tt/1PTl8nh

A chronological listing of the news articles posted on the Skeptical Science Facebook page during the past week.

Sun, Nov 22

Mon, Nov 23

Tue, Nov 24

Wed, Nov 25

Thu, Nov 26

Fri, Nov 27

Sat, Nov 28



from Skeptical Science http://ift.tt/1PTl8nh

Venus and Spica in late November, 2015

Tomorrow before dawn – November 29, 2015 – it’ll be hard to miss the planets Venus and Jupiter blazing away in the sky before sunrise. Venus and Jupiter rank as the third-brightest and fourth-brightest celestial bodies, respectively, after the sun and moon. In the predawn hours, you can also catch Spica, the constellation Virgo’s brightest star, near Venus. After you spot Venus and Spica, think of this. For the rest of your life – every 8 Earth-years (every 13 Venus-years) – Venus and Spica will meet up in this same place in the morning sky. So that’s 2015, 2023, 2031, 2039 and so on.

What’s more, Venus will reach perihelion – its closest point to the sun in its orbit – on November 29, 2015. Venus’ orbit is the closest to being circular of all the planets in our solar system. Its distance from the sun only varies by only about 1.5% between perihelion and aphelion (farthest point from the sun).

Venus is well known for its 8-year cycles. This planet – which orbits the sun one step inward from Earth – swings to perihelion 13 times every 8 years. So Venus’ 13th return to perihelion will happen some 8 years from now – on November 28, 2023 – with Venus and Spica returning to virtually the same spot in the November 2023 morning sky.

Venus returns to perihelion 13 times in 8 years:

1. 2016 July 10
2. 2017 Feb 20
3. 2017 Oct 3
4. 2018 May 16
5. 2018 Dec 26
6. 2019 Aug 8
7. 2020 Mar 20
8. 2020 Oct 30
9. 2021 Jun 12
10. 2022 Jan 23
11. 2022 Sep 4
12. 2023 Apr 17
13. 2023 Nov 28

Almost gone! EarthSky lunar calendars make great gifts. Order now.

Spica, a key star of the Zodiac, serves as a perfect example of a 1st-magnitude star. In other words, Spica is one of the brightest stars in our sky.

Yet Spica pales next to dazzling Venus, which outshines this star by a hundredfold.

You can reliably count on brighter Venus to guide your eye to fainter Spica throughout late November and early December, 2015. When Venus is no longer there for guidance, you can always star-hop to Spica from the constellation Corvus the Crow.

By the way, you can also spot the red planet Mars between Venus and Jupiter, as shown on the chart at the top of this post. The green line on the chart depicts the ecliptic – Earth’s orbital plane projected onto the dome of sky – and thus the sun’s apparent yearly path through the constellations of the Zodiac.

Dates of sun’s entry into each constellation of the Zodiac

Because the planets of our solar system orbit the sun on nearly the same plane as Earth, you know you can always look for planets on or near the ecliptic, or the sun’s annual path in front of the backdrop stars.

Bottom line: Watch for the brilliant planet Venus near the bright star Spica in late November and early December, 2015.

EarthSky astronomy kits are perfect for beginners. Order today from the EarthSky store

Donate: Your support means the world to us



from EarthSky http://ift.tt/1MARaUo

Tomorrow before dawn – November 29, 2015 – it’ll be hard to miss the planets Venus and Jupiter blazing away in the sky before sunrise. Venus and Jupiter rank as the third-brightest and fourth-brightest celestial bodies, respectively, after the sun and moon. In the predawn hours, you can also catch Spica, the constellation Virgo’s brightest star, near Venus. After you spot Venus and Spica, think of this. For the rest of your life – every 8 Earth-years (every 13 Venus-years) – Venus and Spica will meet up in this same place in the morning sky. So that’s 2015, 2023, 2031, 2039 and so on.

What’s more, Venus will reach perihelion – its closest point to the sun in its orbit – on November 29, 2015. Venus’ orbit is the closest to being circular of all the planets in our solar system. Its distance from the sun only varies by only about 1.5% between perihelion and aphelion (farthest point from the sun).

Venus is well known for its 8-year cycles. This planet – which orbits the sun one step inward from Earth – swings to perihelion 13 times every 8 years. So Venus’ 13th return to perihelion will happen some 8 years from now – on November 28, 2023 – with Venus and Spica returning to virtually the same spot in the November 2023 morning sky.

Venus returns to perihelion 13 times in 8 years:

1. 2016 July 10
2. 2017 Feb 20
3. 2017 Oct 3
4. 2018 May 16
5. 2018 Dec 26
6. 2019 Aug 8
7. 2020 Mar 20
8. 2020 Oct 30
9. 2021 Jun 12
10. 2022 Jan 23
11. 2022 Sep 4
12. 2023 Apr 17
13. 2023 Nov 28

Almost gone! EarthSky lunar calendars make great gifts. Order now.

Spica, a key star of the Zodiac, serves as a perfect example of a 1st-magnitude star. In other words, Spica is one of the brightest stars in our sky.

Yet Spica pales next to dazzling Venus, which outshines this star by a hundredfold.

You can reliably count on brighter Venus to guide your eye to fainter Spica throughout late November and early December, 2015. When Venus is no longer there for guidance, you can always star-hop to Spica from the constellation Corvus the Crow.

By the way, you can also spot the red planet Mars between Venus and Jupiter, as shown on the chart at the top of this post. The green line on the chart depicts the ecliptic – Earth’s orbital plane projected onto the dome of sky – and thus the sun’s apparent yearly path through the constellations of the Zodiac.

Dates of sun’s entry into each constellation of the Zodiac

Because the planets of our solar system orbit the sun on nearly the same plane as Earth, you know you can always look for planets on or near the ecliptic, or the sun’s annual path in front of the backdrop stars.

Bottom line: Watch for the brilliant planet Venus near the bright star Spica in late November and early December, 2015.

EarthSky astronomy kits are perfect for beginners. Order today from the EarthSky store

Donate: Your support means the world to us



from EarthSky http://ift.tt/1MARaUo