astronomers are blessed to live in a largely transparent world
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Astronomers are blessed to live in a largely transparent world. While taking that for granted, we’re continually struggling to penetrate the remaining realms of darkness. Southern Summer Nightsky. - PowerPoint PPT PresentationTRANSCRIPT
Astronomers are blessed to live in a largely transparenttransparent world
While taking that for granted, we’re continually struggling to penetrate the
remaining realms of darknessSouthern Summer Nightsky
Earth’s atmosphere is remarkably transparent to visible light,
with a few critical exceptions:
1) Clouds (suspended droplets) can easily block our vision of space.
Nice to have desert mountain ranges,
Lucky we’re not on our sister planet, Venus
0) Scattered light swamps much fainter signal from stars and galaxies:Don’t forget to turn out the lights!
Wish I were HERENot THERE!
Venera lander on gloomy surface of Venus
Earth’s atmosphere is remarkably transparent to visible light,
with a few critical exceptions:
2) Ozone absorbs (lethal) Ultraviolet radiation
(too little transparency would be fatal)
Transparency,
The ratio of the red to the black curves,
is 80% for most visible light
UV, wiped out by O3 IR, Absorbed by H20, C02, CH4
Sunlight, hitting
Sunlight
B G Y R
Earth’s atmosphere is remarkably transparent to visible light,
with a few critical exceptions:
3) Greenhouse molecules absorb Infrared radiation escaping the Earth, keeping our surface above freezing
Nearly every aspect of scientific revolutions, from Galileo to Newton, to Einstein, needed transparent views of the sky, particularly our Solar System
In recent decades, astronomers have spent $Billions$ to get around those 3 obstructions, with special telescopes
in special locations
Next breakthroughs in human perception of the cosmos came because
we can see beyond our Solar System
Very Lucky Most of our Milky Way galaxy is transparent
to visible light
Hercules Deep Field
Milky Way
Was revealed by Galileo’s
telescope to be a
GALAXY of billions
of Suns
But a serious problem is evident: Blue light cannot travel through the
disk of our Galaxy TransparencyTransparency only holds for long
wavelengths, Infrared and Radio
Closer view of the plane of the Milky Way towards Sagitarius,Which systematically absorbs the blue light,But Passes the redder light
This infrared picture (tilted to horizontal) gives much better view ofOur Milky Way galaxy than any visible photograph
Less than 1% of galactic mass is in SOLID form, “dust” grains
the size of the wavelength of visible light
Same effect is seen at sunset
Strong motivation to improve infrared and
radio telescopes
Dusty regions of space are where all stars (and planets) were, and are
formed
On outskirts of Milky Way, we have an unobstructed view out of our
galactic plane
Lucky Deep (intergalactic) Space is almost completely empty
Using large telescopes as time machines,
Milky Way Star (foreground)
In all directions, we see through the foreground of Milky Way stars, to discover an almost endless superposition of galaxies, all the way back to their birth
Hercules Deep Field,a 13-Billion Light-year Needle “drill core” across the history of the Universe, traces most of the evolution of galaxies, from origins to present day
2 minutes of arc (1/30th of a degree) = about 1 million light years across, at typical galaxy distance
Several thousand galaxies are detectable in this little picture, hundred billion over entire sky
Ultimate limit of Universe’s Transparency:
380,000 years after the Big Bang, all atoms were ionized
the resulting free electrons made earlier times in the Universe completely opaque
Milky Way “Baby Picture”
(scattering of light is just as bad as absorbing it)
We have seen that “free electron wall”, it is the Cosmic Microwave
Background Radiation
NASA’sWMAP
Contrast of microwave brightness extremely enhanced, to reveal the 1 in 100,000 density excesses that were to evolve into…Us
Unlike the births of stars, planets or galaxies, the earliest epoch of the Universe will never be visible, at
any wavelength of light
In principle, we will someday observe the earliest moments of the
Big Bang not by detecting its photons, but instead its neutrinos
and gravity waves
They pass transparently through darn near anything
Nearly every aspect of scientific revolutions, from Galileo to Newton, to Einstein, needed transparent views of the sky, particularly our Solar System