A parsec (pc) is a unit of measurement used in astronomy to describe astronomical distances, particularly on cosmic scales. The term "parsec" is actually a contraction of "parallax of one arcsecond," which refers to the method by which this unit of distance is defined. A parsec is defined as the distance at which an object will appear to shift its position by one arcsecond (1/3,600th of a degree) as observed from Earth when the Earth is on opposite sides of its orbit (at an average distance of one astronomical unit, or about 93 million miles) from the Sun.
In more practical terms, a parsec is approximately equal to 3.09 × 10^16 meters or 3.09 × 10^13 kilometers.
To provide a sense of scale, some common astronomical distances expressed in parsecs include:
Parsecs are especially useful for describing distances between stars and galaxies, as astronomical distances can be incredibly vast, and using kilometers or even light-years can lead to unwieldy numbers.
An attometer (am) is an even smaller unit of measurement used to express incredibly tiny distances. It is equal to one quintillionth of a meter, which is 0.000000000000000001 meters or 1 × 10^-18 meters. The prefix "atto" denotes a factor of 10^-18 in the International System of Units (SI).
Attometers are used in the most specialized and precise scientific research, particularly in the field of particle physics and in discussions about fundamental particles. These distances are relevant when studying the properties and interactions of subatomic particles, such as quarks and neutrinos, which have dimensions on the scale of attometers.
To put it into perspective, the size of an attometer is approximately a billion times smaller than the diameter of a hydrogen atom, which is already on the order of picometers. Attometers are among the smallest scales of measurement used in scientific research and are essential for understanding the behavior of matter at the most fundamental level.