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- From: phfrom@nyx.uni-konstanz.de (Hartmut Frommert)
- Subject: Re: Two sticky questions on astrophysics
- Message-ID: <phfrom.388@nyx.uni-konstanz.de>
- Sender: usenet@eratu.rz.uni-konstanz.de
- Organization: Dept. of Physics, University of Constance
- References: <ednclark.721916494@kraken>
- Date: Tue, 17 Nov 1992 10:44:35 GMT
- Lines: 107
-
- Although this belongs to sci.astro or sci.physics (but please don't
- crosspost):
-
- ednclark@kraken.itc.gu.edu.au (Jeffrey Clark) writes:
-
- >1. Nothing can travel faster then the speed of light. Therefore
- >gravitational influence takes time to travel.
-
- Right. An approximate formula for the gravitational potential in the
- linearized, Newtonian (weak field) limit of Einstein theory is
-
- U(r,t) = - G * \int d^3 r' (1/|r-r'|) \rho(r', t - |r-r'|/c)
-
- ("retarded" potential)
-
- >Therefore the influence of
- >objects on the other side of the galaxy are being felt in our solar system
- >as those far flung objects were some 80,000 years ago, yes? More to the
- >point the massive centre of our galaxy (possibly contains a mega-black hole)
- >will not influence us from it's current position for another 30,000 years.
-
- But from the position where it was 30,000 years ago.
-
- >Now this (according to my naive musings) should not present a problem if we
- >are orbiting the centre of our galaxy in a near perfect circular orbit, but
- >I would surmise that our solar system would have some eccentricity in it's
- >orbit. According to me the solar system is falling toward a non-existant
- >centre and has been doing this (as all galactic objects do) since the
- >beginning of galactic history. Should this not cause orbital deviations
- >that are measurable? Can someone help me out here please am I missing some
- >obvious relativistic point?
-
- Of course there are influences on the Sun's orbit around the galaxy. At
- least approximately (i.e. when General Relativity is strictly valid) the Sun
- (and with it the Solar System) is moving along a timelike "geodesic", i.e.
- the straightest possible line in curved spacetime, where the curvature of
- spacetime is caused by the massive bodies in it.
-
- So for now, you can imagine spacetime as a "deformable" substrate, where all
- mass and energy cause thedeformation, i.e. curvature, at the place and time
- (i.e. "event") they are.
- (BTW, this is exactly the physical contents of Einstein field equations.)
- The deformations then propagate with the velocity of light, i.e. spacetime
- is no more a static background, but dynamically influenced by matter. On the
- other hand, matter is "bound" to spacetime, and a particle, or the Sun and
- planets, trying to move as straight as possible, move along geodesics, i.e.
- are effected by the curvature of spacetime, at the place they are.
- (BTW, this is expressed in the equation of continuity for the energy momentum
- tensor in GR).
-
- >2. An object is detected 15 billion light years away, pushing the beginning
- >of time to at least that many years ago. But surely it pushes that time to
- >double 15 billion years (ie 30 billion years).
-
- As nobody has rods to measure the actual distance of the object, one has to
- derive the distance from other features. At that large distances you
- mention, there are (at least to my knowledge) no "standard candles"
- resolvable for telescopes. Instead of a real distance, only the redshift
- of the object is measured. According to Hubble's law of expansion, you may
- then calculate the corresponding distance, depending on the Hubble constant.
- Therefore you can only conclude that the object is seen at a time when the
- universe was, say, 10 % as large as now (it's rather complicated, indeed).
- This may be 15 billion light years in one and 8 billion in another model.
- Thereby you can, of course, never conclude how old the universe is, from the
- distance of objects: The 15 billion years come from the theory of stellar
- evolution (age of globular clusters in our Milky Way galaxy).
-
- BTW: If we knew H_0 we could determine the approximate distance *today*
- from Hubble's law.
-
- >Nothing can travel faster
- >than light.
-
- That is true only locally. But the object observed is (at least
- approximately) at rest locally, i.e. moving at most with some % of light
- velocity with respect to its own neighborhood. Only at the large distance
- it *seems* to move nearly with v=c, because the universe expands. Therefore
- it is well possible that there are regions of the universe that seem to
- escape faster than light from us.
-
- >The object that generated that radiation did so 15 billion years
- >ago from 15 billion light years away. But first we had to get 15 billion
- >light years away from this object. Both the object and the particles that we
- >consist of must have been together at the Big bang. In order for the light
- >to have taken 15 billion years to reach us, the object must have been 15
- >billion light years away from our current position 15 billion years ago. In
- >other words the earth and the object relative to each other must have been
- >travelling for some 15 billion years (at least) to get that far apart before
- >the light was emmitted from far-flung object. Once again am I missing some
- >obvious relativistic point or have I just doubled the age of the universe?
-
- As above, all the events you describe are local, according to GR. The light
- was emitted by the object approx. 15 billion years ago. Then it was moving
- with v=c, getting redder and redder due to cosmic expansion, independent of
- the emitter as well as the observer. At last, after traveling a long time
- and distance, which is difficult to calculate exactly, it arrived at a
- telescope, and we can calculate the distance, etc. from the redshift. That
- we can observe the latter is only possible because the spectra of the
- chemical elements are the same at the place and time of emision in the
- distant object and in Earth based laboratories.
-
- >[...] Depending on the answers I've got some other queries as well.
-
- But please don't post them on sci.space.
- Hartmut Frommert <phfrom@nyx.uni-konstanz.de>
- Dept of Physics, Univ of Constance, P.O.Box 55 60, D-W-7750 Konstanz, Germany
- -- Eat whale killers, not whales --
-