[meteorite-list] OT: HUDF center top left, #90 astrodeep200407aab10ada.png 3.68 MB 1244X1243 1 of 4 identical views with different color schemes 2008.12.12 #88-91 on rmforall at flickr.com: Rich Murray 2011.01.09

From: Rich Murray <rmforall_at_meteoritecentral.com>
Date: Sun, 9 Jan 2011 00:54:56 -0700
Message-ID: <AANLkTikES1Lit+B8Gv5cKsTbno6u9dMho4J0wTop5_aO_at_mail.gmail.com>

OT: HUDF center top left, #90 astrodeep200407aab10ada.png 3.68 MB
1244X1243 1 of 4 identical views with different color schemes
2008.12.12 #88-91 on rmforall at flickr.com: Rich Murray 2011.01.09
http://rmforall.blogspot.com/2011_01_01_archive.htm
Sunday, January 9, 2011
[ at end of each long page, click on Older Posts ]
http://groups.yahoo.com/group/astrodeep/message/80
[you may have to Copy and Paste URLs into your browser]
____________________________________________________________


for viewing -- click on Actions to get different sizes and for free download

http://www.flickr.com/photos/rmforall/3103426063/in/photostream/

#89 astrodeep200407aab10aea.png 4.14 MB 1244X1283 HUDF center top left

This image is 6.3x6.3 arc-seconds, 3.965% of the area of the Hubble
Ultra Deep Field,

which is 186 arc-seconds wide and high = 3.1 arc-minutes

= 1/10 width of the Full Moon or Sun, about 0.5 degrees,

so the HUDF is about 1% of the area of the square that holds the Full
Moon or Sun,

short introduction re viewing lovely subtle earliest structures in
HUDF: AstroDeep, Rich Murray 2009.02.23

I've found since 2005 myriad ubiquitous bright blue sources, always on
a darker fractal 3D web, along with a variety of sizes of irregular
early galaxies, in the Hubble Ultra Deep Field, simply by increasing
the gamma from 1.00 to 2.00 and saturating the colors, while
minimizing the green band to simplify the complex overlays of complex
fractal structures.

Dozens of these images, covering the entire HUDF in eight ~20 MB
segments, are available for viewing at many scales [ To change the
size of images on Windows PCs, use Control - and + ] on www.Flickr.com
at the "rmforall" photostream. Try #86 for the central 16% of the
HUDF.

ubiquitous bright blue 1-12 pixel sources on darker 3D fractal web in
five 2007.09.06 IR and visible light HUDF images, Nor Pirzkal,
Sangeeta Malhotra, James E Rhoads, Chun Xu, -- might be clusters of
earliest hypernovae in recent cosmological simulations: Rich Murray
2008.08.17 2009.01.20
rmforall.blogspot.com/2008_08_01_archive.htm
Sunday, August 17, 2008
groups.yahoo.com/group/AstroDeep/25
groups.yahoo.com/group/rmforall/85

www.flickr.com/photos/rmforall/1349101458/in/photostream/

The 5 closeups are about 2.2x2.2 arc-seconds wide and high, about 70x70 pixels.
The HUDF is 315x315 arc-seconds, with N at top and E at left.
Each side has 10,500x10,500 pixels at 0.03 arc-second per pixel.

Click on All Sizes and select Original to view the highest resolution
image of 3022x2496 pixels, which can be also be conveniently seen
directly at their Zoomable image:

www.spacetelescope.org/images/html/zoomable/heic0714a.html

Notable in the deep background of the five closeups are ubiquitous
bright blue sources, presumably extremely hot ultraviolet before
redshifting, 1 to a dozen or so pixels, as single or short lines of
spots, and a few irregular tiny blobs, probably, as predicted in many
recent simulations, the earliest massive, short-lived hypernovae, GRBs
with jets at various angles to our line of sight, expanding bubbles,
earliest molecular and dust clouds with light echoes and bursts of
star formation, and first small dwarf galaxies, always associated with
a subtle darker 3D random fractal mesh of filaments of H and He atomic
gases.

As a scientific layman, I am grateful for specific cogent, civil
feedback, based on the details readily visible in images in the public
domain.

www.spacetelescope.org/images/html/heic0714a.html

Hubble and Spitzer Uncover Smallest Galaxy Building Blocks

Rich Murray, MA Room For All rmforall at gmail.com 505-819-7388
1943 Otowi Road, Santa Fe, New Mexico 87505
groups.yahoo.com/group/rmforall/messages
groups.yahoo.com/group/AstroDeep/messages
www.sfcomplex.org Santa Fe Complex

You are welcome to visit me and share your comments as I share these
images at home on a 4X8 foot screen -- no fee.

Anyone may view and download for free 91 images, presenting the HUDF
in eight 20 MB pieces at rmforall at www.FlickR.com -- #86 is about
20% of the HUDF in their red and blue colors, as leaving out the green
greatly simplifies interpreting the overlapping layers of transparent
fractal webs of gas with a wide range of sizes of rather distant
sources, beyond z = 5.
_____________________________________________________________


astrodeep200407aab10ada.png 3.10 MB flickr.com rmforall #90
astrodeep200407aab10ada.png 3.68 MB 1244X1243 px HUDF center top left:
Lillian J Kelly: Rich Murray 2008.12.30

The attachment is my image from my hard drive:
astrodeep200407aab10ada.png

www.flickr.com

www.flickr.com/photos/rmforall/3103426063/
#90 astrodeep200407aab10ada.png 3.68 MB 1244X1243 px HUDF center top left

Click on All Sizes to see and download the Original
or find it directly at
farm4.static.flickr.com/3161/3103426063_df229d2202_o.png

In Windows Vista, use CTRL +/= over and over to magnify images,
and CRTL _/- to reduce.

You can also go to Control Panel to Ease of Access
to Ease of Access Center
to Optimize visual display
to turn on Magnifier,
which creates a box of any size and location that magnifies
from 1 to 16 times in width and height,
whatever area the cursor is pointed at on any image on the screen.
You can even make "stereo" pairs side by side,
by setting Magnifier to 1X,
and putting its box to the left or right half of the screen,
and using the cursor to adjust
until the two images are matching and side by side.
Then if you can, gaze with crossed eyes at the two images
to get a third image in between,
which may well look 3D and have much more detail.

This image is 6.3x6.3 arc-seconds, 3.965% of the area of the Hubble
Ultra Deep Field,

which is 186 arc-seconds wide and high = 3.1 arc-minutes

= 1/10 width of the Full Moon or Sun, about 0.5 degrees,

so the HUDF is about 1% of the area of the square that holds the Full
Moon or Sun,

while the image is 4% of 1/1,000 of the area of the HUDF,

so the image is about 4/100,000 of the area of the square that holds
the Full Moon or Sun.

The image is 6.3 are-seconds wide and high,

while the pixels are 0.03 arc-seconds wide in the original HUDF.

The background of many small blue spots are about 1-10 pixels in area.

I have used a simple, low-cost program, MGI PhotoSuite 4.0 to process
these images:

double the Gamma to 2.00,
raise the color saturation,
shift colors a bit to accentuate the reds,
remove most of the Green band,
so the image is mostly made of Blue (coding for visible blue),
with Red codes for the invisible infrared just longer in wavelength
than visible red.

Mixed Blue and Red make green, yellow, orange, red, and white.

However these colors are downshifted in frequency (lengthened in wavelength)
more and more the more they are distant in space (light travel time from us):

The "Little Feller", like the figure "8" in the top center
to the right of the red galaxy with a red swirl on the right,
has been measured to be at redshift distance z = 4.88,
so its light is changed by a factor of 4.88 --
its apparent reds, oranges, and yellows represent radiation in the hot
ultraviolet,
and its age from us is about 13 billion years,
about a billion years after the Big Bang,
13.7 billion = 13,700 million years ago.
The Sun and solar system are 4.6 billion = 4,600 million years ago.

The myriad tiny background blue spots,
along with some green ones,
always on a dark 3D fractal mesh,
are probably the first stars,
made of pure hydrogen and helium,
about 100-100 solar masses in size,
extremely hot and short-lived,
exploding as hypernovae after 1-2 million years,
often with intense bipolar jets,
often leaving relic neutron stars and black holes,
flinging new elements like carbon, nitrogen, and oxygen into space to
become the substance of later generations of stars,
which are closer to us in space (nearer in time), smaller, more
numerous, cooler, longer-lived,
collecting together by gravity to make clouds, clusters, dwarf
galaxies, clump cluster galaxies, irregular galaxies, and mature
galaxies,
flat slowly rotating spirals and rounded ellipticals,
which often collide, especially at first
before the constant expansion of space-time separated them more and more --
the expansion of space-time itself that originated from a minute
region in a source reality
that had at least 10 dimensions of space and one of time -- the Big Bang.

So, we see far-away early gatherings of hot blue and green objects,
and closer (nearer to us in time) more numerous gatherings of cooler
red objects,
which all seem exist as a 3D fractal network of twisted tubes,
rather transparent, as there was little dust in early time to darken light.

It is well known that for every mass of ordinary matter, gas, dust, stars,
there is about 6 times more mass of completely invisible dark matter,
which pulls itself together by gravity into a 3D fractal network, making
the scaffold that ordinary matter collects within.
Dark matter surrounds glalaxies and superclusters of galaxies,
bending light gently by gravity,
so that the dark matter appears as subtle transparent bubbles
against the complex background of deeper structures.

Additionally the cosmic zoo may include galaxy-wide strings of
condensed space-time geometry, formed during the Big Bang,
that are massive enough to bend light
and make double twin images of objects far behind them from us.

ubiquitous bright blue 1-12 pixel sources on darker 3D fractal web in
five 2007.09.06 IR and visible light HUDF images, Nor Pirzkal,
Sangeeta Malhotra, James E Rhoads, Chun Xu, -- might be clusters of
earliest hypernovae in recent cosmological simulations: Rich Murray
2008.08.17
rmforall.blogspot.com/2008_08_01_archive.htm
Sunday, August 17, 2008
groups.yahoo.com/group/AstroDeep/25
groups.yahoo.com/group/rmforall/85

... [ more ]
____________________________________________________________


Rich Murray, MA Room For All rmforall at gmail.com
505-819-7388 1943 Otowi Road Santa Fe, New Mexico 87505

groups.yahoo.com/group/rmforall/messages

groups.yahoo.com/group/AstroDeep/messages

www.sfcomplex.org Santa Fe Complex
____________________________________________________________
Received on Sun 09 Jan 2011 02:54:56 AM PST