Stereoscopic deep space imaging

In summary, Bob has a new idea for creating deep space stereoscopic images. His calculations predict that it would be possible to create images of distant stars with a precision of 156 ly. However, he cautions that this would only be useful for a select few stars. Gaia, a forthcoming space telescope with a goal of positional accuracy of 24 µas, may be able to achieve this level of accuracy for most of the stars in our galaxy.
  • #1
Bob__
7
0
Hello people, first i need to say that i am quite a newb for astronomy.
I have a idea about creating deep space stereoscopic images.
I was wondered if it is usable to place two satellites(space telescopes) in heliocentric orbit, with distance approximately that of pluto , that are 180 degrees one from another - each on a different side of the sun. They would simultaneously take pictures of same sectors of space, thus creating a stereoscopic image of a star cluster, planetary system or whatever.
I have calculated that this could create valuable stereo-images , by analogy of my stereoscopic view.
I can clearly distinguish image dept at 10 km distance with my eyes, so i divided that distance with the distance between my eyes - 10km/6cm = 166666.666
166666.666*(29.657*2) AU(pluto perihelion) =9.88566663e+06
9.88566663e+06 /63241 AU(light year)= 156.31 light years.

29.657*2 - pluto perihelion *2 - distance between the satellites
all astronomical distances are in AU


I think that dept perception can be distinguished even at distances greater then 10 km for human eye, and computer vision is clearly superior and more sensitive then the human eye.
Still even if it is just 156 ly, there are thousands of stars to observe.
Are my calculations valid?
And could this idea be somehow useful for astronomy?
 
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  • #2
Hi Bob, welcome to PF!

What you're talking about is called parallax, and is routinelly used to determine distances to nearby stars. Rather than facing the technological challenges involved in placing telescopes in deep space, astronomers tend to use the convenient natural solar satellite - the Earth. By making observations of a given objects at two times, half a year apart, they can observe the parallactic displacement of the target with respect to the so called "background stars". Earth's orbit only gives you 2AU triangulation base, but you should see how the loss of accuracy over your ~60 AU proposition is outweighed by the convenience factor.

Wiki has got a nice article on the subject:
http://en.wikipedia.org/wiki/Parallax
 
  • #3
It is possible to get more accurate observations from space, but there's no need to send a satellite very far as the Earth itself moves to either side during the year.

The Hipparcos satellite made parallax and proper motion observations of this type from Earth orbit. (It was intended to go into geostationary orbit, but ended up in a transfer orbit instead, but was still able to achieve its mission objectives).
 
  • #4
Of course there is only a handful of stars close enough to have measurable parallax. For the vast majority of stars this would not help much if at all.
 
  • #5
Yeah... Parallax , i have forgotten that term
well Wikipedia sort of answered my questions.
Given a second thought , it is not so bright idea to send two satellites on a 12 year trip to function for a perhaps half of that time, given that Hubble space telescope was regularly repaired.
And 2 AU or 60 AU is not as essential as i previously thought.
Thanks for the help ppl :)
 
  • #7
Integral said:
Of course there is only a handful of stars close enough to have measurable parallax. For the vast majority of stars this would not help much if at all.

The Hipparcos satellite measured the parallax of over 50,000 stars. I guess this is a "handful" if you have big hands! The Gaia satellite, set to launch soon, will extend this to a billion stars. Parallax measurements just keep getting better. Gaia has a goal of positional accuracy of 24 μas, which is the parallax of an object at about 100,000 light-years distance. This is most of the stars in our galaxy.
 
  • #8
Integral said:
Of course there is only a handful of stars close enough to have measurable parallax. For the vast majority of stars this would not help much if at all.

You underestimate today's optics, CCD's, and the clarity afforded by being in space. Read up about Gaia mission. ~15 µas precision for stars with magnitude 15 and less!
 

1. What is stereoscopic deep space imaging?

Stereoscopic deep space imaging is a technique used to capture three-dimensional images of objects in outer space. It involves taking two or more images from slightly different angles and then combining them to create a 3D image.

2. How is stereoscopic deep space imaging different from regular imaging?

In regular imaging, only one image is captured, while in stereoscopic deep space imaging, multiple images are taken at different angles. These images are then combined to create a 3D effect, allowing for a more immersive viewing experience.

3. What is the purpose of using stereoscopic deep space imaging?

Stereoscopic deep space imaging allows scientists to gain a better understanding of the structure and depth of objects in space. It also helps in creating more accurate and detailed models of celestial bodies.

4. What equipment is needed for stereoscopic deep space imaging?

To capture stereoscopic deep space images, specialized cameras with dual lenses or multiple cameras are needed. Additionally, precise positioning and calibration of the cameras are crucial for creating high-quality 3D images.

5. Can stereoscopic deep space imaging be used for studying all objects in space?

Yes, stereoscopic deep space imaging can be used to study a wide range of objects in space, including planets, stars, galaxies, and other celestial bodies. It is especially useful for studying objects that have complex and irregular shapes.

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