Can Optical Interferometers Extend Beyond 1 Light Second in Length?

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In summary, there is currently no active space interferometry mission and none of the proposed missions have been realized. However, LISA was originally planned with a 5 million km baseline and can still achieve interferometry over a distance of 10 light seconds. The density of the solar wind at 1 AU is significantly lower than the Earth's atmosphere, reducing the potential for interference. However, sparse interferometers may still have side-lobes that can affect the accuracy of the resolution.
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smartalek86
Is there a limit to optical space interferometry? I read this article
https://www.noao.edu/meetings/interferometry/workshop-files/Carpenter-Space-comp.pdf about future concepts(which i think is really good). I'm wondering, can optical interferometers have a length of more than 1 light second...could you place 3 say in the asteroid belt and have a 2 AU resolution
 
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None of the proposed missions there was realized, and there is no space interferometry mission actively in preparation (unless you count LISA Pathfinder / LISA).

LISA was originally planned with 5 million km baseline, as NASA stopped contributing ESA scaled it down to 3 million km (10 light seconds), so you can do interferometry over these distances.

The solar wind at 1 AU is 19 orders of magnitude less dense than the atmosphere, 100 million km in space have the same area density as 100 nm of (sea level) air, so I wouldn't expect problems from seeing.

Very sparse interferometers tend to have significant side-lobes - you get a good resolution at the place you are looking at, but you also get light from elsewhere.
 
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FAQ: Can Optical Interferometers Extend Beyond 1 Light Second in Length?

What are interferometers and how do they work?

Interferometers are scientific instruments that use the principle of interference to measure and study light, sound, or other types of waves. They work by splitting a beam of light or other wave into two or more parts, then recombining them to create an interference pattern that can be analyzed.

What are the limitations of interferometers?

One of the main limitations of interferometers is that they are sensitive to external disturbances, such as vibrations or changes in temperature. This can affect the accuracy and precision of the measurements. Additionally, the size and weight of interferometers can also limit their portability and practicality for certain applications.

How do we overcome the limitations of interferometers?

To overcome the limitations of interferometers, scientists use various techniques such as isolating the instrument from external disturbances, using advanced stabilization methods, and improving the materials and design of the instrument. Additionally, advancements in technology have allowed for the development of smaller and more portable interferometers.

What types of measurements can interferometers be used for?

Interferometers can be used for a wide range of measurements, including distance, displacement, velocity, and angular rotation. They are also used in fields such as astronomy, metrology, and optical testing, to study and measure phenomena such as gravitational waves, surface roughness, and the properties of materials.

What are some recent advancements in interferometry?

Recent advancements in interferometry include the development of ultra-stable interferometers, which can measure tiny changes in distance with extreme precision. There have also been advancements in the use of interferometers in gravitational wave detection, allowing for the observation of previously undetectable phenomena in the universe.

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