From: Greg Neill on
Brad Guth wrote:
> On Apr 23, 5:09 am, "Greg Neill" <gneil...(a)MOVEsympatico.ca> wrote:
>> Brad Guth wrote:
>>> On Apr 22, 1:33 pm, "Greg Neill" <gneil...(a)MOVEsympatico.ca> wrote:
>>>> Brad Guth wrote:
>>>>> How about photons from a vibrant 10 solar mass star that's situated
>>>>> well within our visual detection horizon of 13.7e9 ly, but trekking
>>>>> directly towards us at -c?
>>
>>>> It can't. Nothing physical within our horizon can be
>>>> observed to move at or above c. Close to c, sure, but
>>>> not at or above.
>>
>>>> The best a body can do is approach c with respect to
>>>> observers in its proximity (within the local region of
>>>> space moving with the Hubble flow). Every non-local
>>>> observer (such as us sitting a great distance away from
>>>> that region in our own local region) sees that region
>>>> of space moving away in bulk according to the Hubble
>>>> expansion, thus decreasing any net speed of approach.
>>
>>> I wasn't asking for your subjective opinion of physics.
>>
>>> I was asking about photons from a vibrant 10 solar mass star that's
>>> situated well within our visual detection horizon of 13.7e9 ly,
>>> trekking directly towards us at -c. How would we ho about detecting
>>> this 100% blue-shift?
>>
>> See my first paragraph above.
>>
>> If your observed star is relatively close by, it's observed
>> velocity will be limited by an upper bound approaching c.
>> The further away it is (and the closer it gets to our
>> cosmic horizon), the motion due to the expansion of the
>> space between us and it has to be added to its motion
>> through space, decreasing the net observed velocity.
>>
>> Near the horizon, a body moving at near c in its local space
>> in a direction towards us will have a net velocity near
>> zero (the best it could do would be to stand still with
>> respect to us), and so its red shift would be very small.
>>
>> There is no way for a body to be observed moving towards us
>> at c.
> That's exactly what I�d thought. If we're moving away or towards
> other mass at c, we'd be oblivious to realizing its existence.

I don't see why you persist in assuming the impossible.
A relative velocity of c or greater is simply not allowed
by nature.

>
> I understand there's a few rogue stars moving at 1500 km/sec, and it's
> thought possible that stars further out could easily be moving at .5c,
> so what if another star were moving towards the other at .5c, making
> their mutual closing velocity c. Due to their relative closing
> velocity being c, could either of those fast moving stars notice the
> other? (I don't think so)

Look up relativistic addition of velocities.

Closing velocity, as judged by a third party observer of two
separate objects closing on each other, is not at all the
same thing as one object moving at c or greater with respect
to the other; Each of the stars would see the other as moving
towards it at a velocity less than c. Neither star would be
invisible to the other.

>
> It seems anything moving away or towards us at c (relative to us)
> becomes stealth/invisible.

But nothing can so move. So your conclusions are not logical.

> This simply means we�re always at some
> degree of risk unless fast moving exogravity can be detected. A
> neutron star or black hole closing in on us, even if it were passing
> outside of Pluto could be a cosmic form of fatal attraction, whereas
> just the gravitational shockwave of one light year radii alone could
> perturb and/or traumatize most everything about our solar system.

And invisible pink elephants are a threat to ants of the
13th dimension. Makes as much sense.


From: BURT on
On Apr 22, 4:10 pm, spudnik <Space...(a)hotmail.com> wrote:
> there is no direct observation of "moving away;"
> it is all presupposition of a "Dopplerian" redshift (probably
> related to a belief in Pascal's absolute vacuum; I mean,
> he did do the experiment).

If light is absorbed sideways to motion instead of head on what kind
of energy shift will it have?

Mitch Raemsch
From: spudnik on
that might affect the relative polarization of the wave.

many high-energy astrophysical experiments do not bother
wtih polarization, even though that's just about all
that there is to "see."

> If light is absorbed sideways to motion instead of head on what kind
> of energy shift will it have?
From: BURT on
On Apr 22, 5:13 pm, spudnik <Space...(a)hotmail.com> wrote:
> that might affect the relative polarization of the wave.
>
> many high-energy astrophysical experiments do not bother
> wtih polarization, even though that's just about all
> that there is to "see."
>
>
>
> > If light is absorbed sideways to motion instead of head on what kind
> > of energy shift will it have?- Hide quoted text -
>
> - Show quoted text -

If from ahead or behind there is an energy shift what about sideways
absorption of light?

It looks as if angle determines the energy shift. With a maximum, and
a zero for 90 degrees to motion.

Mitch Raemsch
From: Brad Guth on
On Apr 22, 1:33 pm, "Greg Neill" <gneil...(a)MOVEsympatico.ca> wrote:
> Brad Guth wrote:
> > How about photons from a vibrant 10 solar mass star that's situated
> > well within our visual detection horizon of 13.7e9 ly, but trekking
> > directly towards us at -c?
>
> It can't.  Nothing physical within our horizon can be
> observed to move at or above c.  Close to c, sure, but
> not at or above.
>
> The best a body can do is approach c with respect to
> observers in its proximity (within the local region of
> space moving with the Hubble flow).  Every non-local
> observer (such as us sitting a great distance away from
> that region in our own local region) sees that region
> of space moving away in bulk according to the Hubble
> expansion, thus decreasing any net speed of approach.

I wasn't asking for your subjective opinion of physics.

I was asking about photons from a vibrant 10 solar mass star that's
situated well within our visual detection horizon of 13.7e9 ly,
trekking directly towards us at -c. How would we ho about detecting
this 100% blue-shift?

~ BG