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originally posted by: toysforadults
a reply to: roadgravel
Why don't you do us a favor and explain the difference between both of the process rather than throw out that strawman?
originally posted by: carewemust
originally posted by: Kandinsky
a reply to: carewemust
If you squint, there's a little alien bastard waving the bird at us.
What sector? Seriously, if you can see individual stars in another galaxy, finding ancient ruins, or crash sites in our solar system should be a snap.
originally posted by: carewemust
a reply to: sputniksteve
Thank-you! Now I understand. The telescope is designed like a pair of high-powered binoculars. No matter how you adjust them, you can't see the bump on your wife's butt when she's in the same room with you. Just a big blur. Got it!
originally posted by: SanitySearcher
a reply to: OrionHunterX
And we get told that it was all caused by a big bang of nothing by nothing from nothing into this?
originally posted by: OrionHunterX
originally posted by: SanitySearcher
a reply to: OrionHunterX
And we get told that it was all caused by a big bang of nothing by nothing from nothing into this?
Quantum equations suggest the Big Bang never happened!! We're probably getting back to the old Steady State theory!
originally posted by: sputniksteve
originally posted by: OrionHunterX
originally posted by: SanitySearcher
a reply to: OrionHunterX
And we get told that it was all caused by a big bang of nothing by nothing from nothing into this?
Quantum equations suggest the Big Bang never happened!! We're probably getting back to the old Steady State theory!
I am unfamiliar. Can you possibly link what you are reading for that? Not that I doubt, I just want to read for myself because I am very interested.
It was shown recently that replacing classical geodesics with quantal (Bohmian) trajectories gives rise to a quantum corrected Raychaudhuri equation (QRE). The second order Friedmann equations from the QRE are derived, and show that this also contains a couple of quantum correction terms, the first of which can be interpreted as cosmological constant (and gives a correct estimate of its observed value), while the second as a radiation term in the early universe, which gets rid of the big-bang singularity and predicts an infinite age of our universe.
originally posted by: DanielKoenig
every 'smallest unit of time' each star in the galaxy is emitting a shockingly large burst of energy, a constant stream, and light travels fast and this case relatively continuously, so light from t1 light from t2 light from t3 light from t4 light from t5 of the same star, continuously , so when they have a detector aimed at this galaxy, from each star the light hits the detector at that splittest second boomboomboomboomboom: my question is, how is it not known that some 'orbs' in that image are not the same star 5 or less or more times imprinted, making it seem potentially like there are 5x or less or more amount of visible star orbs visible?
When Hubble beams down images, astronomers have to make many adjustments, such as adding color and patching multiple photos together, to that raw data before the space observatory's images are released to the public.
Hubble doesn't use color film (or any film at all) to create its images. Instead, it operates much like a digital camera, using what's called a CCD (charge-coupled device) to record incoming photons of light. [Spectacular Photos From The Revamped Hubble Space Telescope]
Hubble's CCD cameras don't measure the color of the incoming light directly. But the telescope does have various filters that can be applied to let in only a specific wavelength range, or color, of light.
originally posted by: Lanisius
Hate to burst your bubble but the pic is fake. NASA enhances these photos before release.
originally posted by: Lanisius
Hate to burst your bubble but the pic is fake. NASA enhances these photos before release.
Hubble's CCD cameras don't measure the color of the incoming light directly. But the telescope does have various filters that can be applied to let in only a specific wavelength range, or color, of light.