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Archive for September 29th, 2006

Redshift - recessional velocity or?

Posted by Pelgrim on 29th September 2006

What is redshift?
If the lines in the spectrum of the light from a star or galaxy appear at a lower frequency (shifted toward the red) than where they are observed in the spectrum of the Sun, we say this object has “positive redshift”. The accepted explanation for this effect is that the object must be moving away from us. This interpretation is drawn by analogy with the downward shift in the pitch of a train whistle as it passes through a railroad crossing and then speeds away from us. The question is: “Is recessional velocity the only thing that can produce a redshift, as modern astrophysicists presume?” It has become clear that the answer to that question is an emphatic “NO!”

If the wavelength of an absorption line in an object’s observed spectrum appears at a wavelength that is, say, 1.56 times its “normal wavelength” (the wavelength at which it is observed in a laboratory experiment here on Earth), then we say this object has a “positive redshift of z = 0.56″. The “z value” is simply the observed fractional increase in the wavelength of the spectral lines. The accepted interpretation of this is to say that this object must therefore be receding from us at 56% of the speed of light or 0.56 x 300,000 km/sec. Mainstream astrophysicists believe that recessional velocity, v = cz. This object, therefore, must be very far away from Earth.

But a high redshift value does not necessarily mean the object is far away. There is another, more important cause of high redshift values.

Inherent Redshift
Arp believes that the observed redshift value of any object is made up of two components: the inherent component and the velocity component. The velocity component is the only one recognized by mainstream astronomers. The inherent redshift is a property of the matter in the object. It apparently changes over time in discrete steps. He suggests that quasars are typically emitted from their parent galaxies with inherentiredshift values of up to z = 2. They continue to move away, with stepwise decreasing inherent redshift. Often, when the inherent redshift value gets down to around z = 0.3, the quasar starts to look like a small galaxy or BL Lac object and begins to fall back, with still decreasing redshift values, toward its parent. He has photos and diagrams of many such family groupings. Any additional redshift (over and above its inherent value) is indeed indicative of the object’s velocity. But the inherent part is an indication of the object’s youth and usually makes up the larger fraction of a quasar’s total redshift.

http://www.electric-cosmos.org/arp.htm

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