Re: APOD: The Leo Triplet Galaxies from VST (2011 Aug 03)
Posted: Wed Aug 03, 2011 5:09 pm
ATTN neufer jerrythebiker took you for a ride to Mar 6, 09 APOD. I hope he was sober.
APOD and General Astronomy Discussion Forum
https://asterisk.apod.com/
We can be sure that three galaxies are in the same physical area, because they show quite similar redshifts, generally between 700 and 800 kilometers per second. That is to say, all three galaxies are moving away from us at a velocity of between 700 and 800 kilometers per second. Because space is expanding and carrying its galaxies with it, and because expansion-induced velocities of galaxies correspond to given distances from us (more or less), we can be quite confident that the Leo Triplet galaxies are at similar distances from us. They are about 30 million light-years away, as the caption of today's APOD pointed out.nobby wrote:NGC 3628 seems to be about twice as big as the other two, which to a novice like me would mean that it was either twice as big or much closer. Can someone please explain why they are judged to be in the same physical area?
APOD: The Tidal Tail of NGC 3628 (2007 Jul 27)Ann wrote:Look at this image of the Leo Triplet, which you could see if you followed one of the links of today's APOD
APOD: Sideways Galaxy NGC 3628 (2008 May 15)Ann wrote:A tidal tail like the one belonging to NGC 3628 is an almost sure sign of interaction. So NGC 3628 is interacting with one or more other galaxies
http://asterisk.apod.com/viewtopic.php?f=31&t=24664Ann wrote:Take a look at interacting galaxies NGC5394 and NGC5395, one big and one small:
The picture is by Alex Cherney, amateur astrophotographer, and Noel Carboni, astroimage processing expert from ProDigital Software. Surely Noel Carboni must be "our" Noel C? Congratulations, Noel, on helping Alex Cherney produce such a fine picture of interacting galaxies!
I will assume, from your tag, you are Philip Perkins from Astro Cruise.pgp566 wrote:Well, OK but you don't need a multi-million dollar facility in the Atacama desert - a humble amateur can do this with just as much quality and better colour rendition from his back garden - though this example is downscaled - I will dig out the master image...
http://www.astrocruise.com/galaxies/LeoTrio_07.htm
In the meantime here is a precursor showing the 'duo' part of it:
http://www.astrocruise.com/galaxies/M65-M66_110402.htm
Yes, that's me - thanks! That image is the clearest ever taken of those two galaxies. Not surprising, given it was captured through the world's largest telescope! What a thrill to have the opportunity to work with that data.Ann wrote:The picture is by Alex Cherney, amateur astrophotographer, and Noel Carboni, astroimage processing expert from ProDigital Software. Surely Noel Carboni must be "our" Noel C? Congratulations, Noel, on helping Alex Cherney produce such a fine picture of interacting galaxies!
It's one of several pairs of astoid trails: the red/magenta pairing shows that these were consecutive exposures. Elsewhere in the image there are isolated green trails, these coming from an image exposed at another time. I thought the magenta colour was just my work monitor, which has a distinct warm bias, but now I see it is just the strange palette that ESO have used.n8zrj wrote:Does anyone know what the interloper is to the left of the lower right galaxy (M66)? There is a small red streak followed by a purple streak.
That should, of course, be asteroid...ozalba@aapt.net.au wrote:It's one of several pairs of astoid trails...
Guilty as charged!bystander wrote: I will assume, from your tag, you are Philip Perkins from Astro Cruise.
Agreed, but there wasn't much science in that particular image from the Atacama desert was there? Wasn't it just as much a 'pretty picture' as most amateur images, taken with a few million dollars less outlay, and with rather better colour balance? Gravitational interactions are mentioned of course, but they are referenced just as much, and are more clearly visible, in many amateur images. As you've probably deduced, there are two latent thoughts in this:bystander wrote:I will agree that 'you don't need a multi-million dollar facility in the Atacama desert" just to take pretty pictures (and you do have some), but can you do important science from your back garden?
Preference? What are you talking about? Whose preference? "Using" for what?pgp566 wrote: 2. A preference for using 'professional' images over amateur images even though many of the latter provide _much_ better illustrations of gravitational interaction.
The science performed at 'professional' observatories is their primary mission. The 'pretty pictures' are just an added bonus.pgp566 wrote: Agreed, but there wasn't much science in that particular image from the Atacama desert was there? Wasn't it just as much a 'pretty picture' as most amateur images, taken with a few million dollars less outlay, and with rather better colour balance? Gravitational interactions are mentioned of course, but they are referenced just as much, and are more clearly visible, in many amateur images. ...
Wasn't producing this kind of result something of waste of taxpayer money when much better can be produced by amateurs at NO cost to the taxpayer at all?
Thanks, Ann!n8zrj ยป Wed Aug 03, 2011 7:44 am
Does anyone know what the interloper is to the left of the lower right galaxy (M66)? There is a small red streak followed by a purple streak.
Very much closer to home, this image also contains the tracks of several asteroids within the Solar System that have moved across the images during the exposures. These show up as short coloured lines* and at least ten can be seen in this picture. As Leo is a zodiacal constellation, lying in the plane of the Solar System, the number of asteroids is particularly high.
This image is a composite created by combining exposures taken through three different filters. Light that passed through a near-infrared filter was coloured red, light in the red part of the spectrum is coloured green, and green light is coloured magenta.
These are either green or pairs of magenta/red trails. This is because the exposures used to make the green channel of the final colour image were taken on a different night to those used for the red and magenta, which were taken in sequence on the same night.