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Standard ruler
Astronomical object of known size
Astronomical object of known size
A standard ruler is an astronomical object for which the actual physical size is known. By measuring its angular size in the sky, one can use simple trigonometry to determine its distance from Earth. In simple terms, this is because objects of a fixed size appear smaller the further away they are.
Measuring distances is of great importance in cosmology, as the relationship between the distance and redshift of an object can be used to measure the expansion rate and geometry of the Universe. Distances can also be measured using standard candles; many different types of standard candles and rulers are needed to construct the cosmic distance ladder.
Baryon acoustic oscillations are considered to be essential standard rulers for measuring large-scale structures in the universe.
Relationship between angular size and distance
The relation between the angular diameter (θ), actual (physical) size (r), and distance (D) of an object from the observer is given by:
: D \approx \frac{r}{\theta}
where θ is measured in radians.
Because space is expanding, there is no single unique way of measuring the distance between source and observer. The distance measured by a standard ruler is known as the angular diameter distance. Standard candles measure another type of distance called the luminosity distance.
References
References
- Schirber, Michael. (26 September 2019). "A Cosmic Ruler at 21 Centimeters". [[American Physical Society]].
- Young, Monica. (8 January 2015). "BOSS: A Ruler to Measure Them All". [[Sky & Telescope]].
- Percival, Will. (28 March 2019). "Making cosmological measurements with standard rulers and standard shapes". [[University of British Columbia]].
- de Grijs, Richard. (2011). "An Introduction to Distance Measurement in Astronomy". [[Wiley (publisher).
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