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yourignoranceisbliss
reply to post by skyblueworld
I'm afraid "Deny Ignorance" has become "Stick your head in the sand".
Here's a close-up view of OP's picture.
Now let's wait for the very same serial debunkers to repeat themselves and ad hominem until they're blue in the face.
This deserves a explanation, a bouble leaving the sun? anybody have exampels of this from earlier?
Phage
reply to post by Curious69
This deserves a explanation, a bouble leaving the sun? anybody have exampels of this from earlier?
people.hao.ucar.edu...
people.hao.ucar.edu...
phys.org...edit on 12/4/2013 by Phage because: (no reason given)
skyblueworld
Taken by Richard Schmidt on December 1, 2013 @ Burleith Observatory, Washington, DC.
Details:
While imaging sunspots we observed a fast-moving satellite with a long boom arm crossing the field of view. This sequence spans 36 milliseconds of real time. The object was moving East at 1 degree per second. Lunt LS100 solar telescope.
Link to source on spaceweather.com
Since most satellites move east (more or less) the direction isn't a problem.
This sequence spans 36 milliseconds of real time. The object was moving East at 1 degree per second. Lunt LS100 solar telescope."
Phage
reply to post by ikonoklast
Since most satellites move east (more or less) the direction isn't a problem.
This sequence spans 36 milliseconds of real time. The object was moving East at 1 degree per second. Lunt LS100 solar telescope."
Let's start by guessing that the object is a satellite and it's in an orbit 250 miles above the Earth. That gives it a speed of 17,157 mph (4.76 mi/sec). At that altitude 4.76 miles has an angular length of 1.09º when directly overhead. For an angular velocity of 1.09º/sec.
Now, we don't know the elevation of the Sun at the time (or do we?) and that "1º/sec" is a suspiciously round number but the lower the orbit, the faster and there are satellites which orbit lower than that so, a satellite is entirely plausible and is the likely culprit and prime suspect.
edit on 12/4/2013 by Phage because: (no reason given)
Phage
reply to post by ChuckNasty
Would you care to show your work?
You can start here. A simple way to calculate angular dimensions.
Calculate angle by using a distance of 250 (miles away) and a size of 4.76 (miles per second).
www.1728.org...edit on 12/4/2013 by Phage because: (no reason given)
No. It's the observed angular velocity...how fast it was moving across the sky. Astronomers do not make observations from the center of the planet.
Astronomical terms, 1 deg is with the center of the planet being the center and not the observers altitude.
Phage
reply to post by ChuckNasty
No. It's the observed angular velocity...how fast it was moving across the sky. Astronomers do not make observations from the center of the planet.
Astronomical terms, 1 deg is with the center of the planet being the center and not the observers altitude.
But I'm old. What do I know?
edit on 12/4/2013 by Phage because: (no reason given)
Phage
reply to post by ChuckNasty
The Sun is about 0.5º across.
But by knowing the tracking rate and direction of the telescope and analyzing the pics it wouldn't be too difficult to come up with an accurate angular velocity. That's how they figure out where comets are going, after all, but with a lot more than just "1º/sec east".
I'm just suspicious of such round numbers. 1 is too round for comfort but close enough that it's nothing really unusual.
edit on 12/4/2013 by Phage because: (no reason given)
Phage
At 75,000 feet that comes to 892 mph.
At 20,000 feet: 238 mph.
At 5,000 feet: 59 mph
alfa1
Phage
At 75,000 feet that comes to 892 mph.
At 20,000 feet: 238 mph.
At 5,000 feet: 59 mph
As mentioned earlier, I did my own calculation of the speed based on an image of the sun on that day and used the sunspot group as a reference for the movement of the object.
I got 0.476 degrees/second.
So the speed figures you have are really only half...
At 75,000 feet that comes to 425 mph.
At 20,000 feet: 113 mph.
At 5,000 feet: 28 mph
I'd like it if somebody could check my work.
Taking an approximation of half a degree for the sun