You need to measure it with something flexible, like a string.If you know for sure it is a circle, it would be easier to measure the diameter, then multiply by pi.
The difference between an actual correct view and a displaced visual parallax error
Depends on what measurement standard you are using and what field you are referring to. It is easier tlo measure in kilograms because it involves smaller numbers. However, if you were studying astronomy, you would likely measure the dog in grams, or solar masses.
Yards. Lakes are pretty big, and yards is a larger measurement than feet so yards would be an easier measurement.
It's probably easier to measure the diameter, i.e., the distance across. Measure that, and divide by 2.
Earth isn't a star and doesn't (can't) have a parallax, becuse we use Earth's orbit as a baseline to measure parallax.
A parallax is hard to measure if it is very small - and this happens when the corresponding object is very far away.
The farther the object, the smaller its parallax. In this case, the parallax is about 1/300,000 of an arc-second (and an arc-second is 1/3600 of a degree) - way too small to measure. Perhaps you will eventually find a way to measure smaller parallax angles.
Parallax bars are used in photogrammetry and remote sensing. with the use of the principles of parallax and refraction, parallax bars are used to measure the heights of buildings and other features.
At farther distances, the parallax becomes too small to measure accurately. At a distance of 1 parsec, a star would have a parallax of 1 second (1/3600 of a degree). (The closest star, Toliman, is a little farther than that.) At a distance of 100 parsecs, the parallax is only 1/100 of a second.
A parallax bar is used in surveying to measure horizontal distances and elevations. It typically consists of a bar with two telescopes at each end that can be used to accurately measure distances by taking line of sight readings.
The parallax refers to the apparent change in the star's position, due to Earth's movement around the Sun. This parallax can be used to measure the distance to nearby stars (the closer the star, the larger will its parallax be).
It means that the distance is greater than a certain amount - depending on how precisely you can measure the parallax.
Parallax
Parallax
Parallax measurements rely on observing the apparent shift of a nearby star against a distant background as the Earth orbits the Sun. The angles involved are typically too small to accurately measure in the case of galaxies due to their vast distances. Galaxies are so far away that any parallax shift would be extremely minute and challenging to detect accurately.
Better depth perception.