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Time in physics

physical science Maturity 13-18 Next article →

In physics, time is defined by its measurement. This means that time is essentially what a clock reads. Scientists treat time as a fundamental quantity, much like mass, length, or electric charge. It is a scalar quantity, which means it is a value that does not depend on direction. Time can be used mathematically to understand other important concepts. For example, it helps scientists calculate motion, kinetic energy, and time-dependent fields. Timekeeping is a complex mix of science and technology. It also serves as a vital foundation for all human recordkeeping.

Pendule de Foucault
Pendule de Foucault

Before modern clocks existed, people relied on natural physical processes to mark time. These processes were understandable to every civilization. For example, ancient people watched for the first appearance of the star Sirius. This helped them predict the yearly flooding of the Nile. Others observed the regular cycle of night and day. Farmers used the position of the sun in the sky to mark their work. They watched the sun rise at dawn and reach its highest point at noon. To do this, they often used a gnomon, which is a simple stick that casts a shadow. By measuring the length of this shadow, they could determine the time of day.

Andromeda galaxy Ssc2005-20a1
Andromeda galaxy Ssc2005-20a1

Humanity has developed many different ways to track the passage of time. In ancient Mesopotamia, astronomers recorded the stars using only their naked eyes over 3,500 years ago. This changed in 1609 when Galileo Galilei began using a telescope. This new tool allowed for much more precise observations. Eventually, mechanical clocks began to appear. In the 1300s, Richard of Wallingford built a complex mechanical clock that worked like an astronomical orrery. As technology improved, clocks used ratchets and gears to display time. These machines grew smaller over time. Eventually, they became personal pocket watches that families could own. Later, pendulum clocks became common in the 18th and 19th centuries.

Relativity of Simultaneity
Relativity of Simultaneity

Today, our most accurate timekeeping relies on atomic physics. In the International System of Units, the standard unit of time is the second. Since 1967, the second has been defined by the radiation of a caesium 133 atom. Specifically, it is the duration of the transition between two hyperfine levels of the atom's ground state. This is measured using a caesium atomic clock. These clocks became practical for scientific use after 1955. The current worldwide time standard, known as UTC, is an atomic time standard. It is incredibly precise. Its accuracy is about 10⁻¹⁵ seconds. This means it would only lose one second every 30 million years.

WMAP
WMAP

Our scientific understanding of how time works has shifted significantly over the centuries. For a long time, scientists like Galileo and Isaac Newton believed time was absolute. Newton described time as a universal clock that flows steadily for everyone. He believed time was a linear parameter that moved the same way regardless of external factors. However, Albert Einstein changed this with his theory of relativity. Modern physics shows that time and space are actually merged into a single fabric called spacetime. In this view, time is a coordinate rather than just a background timeline. Rates of time can actually change depending on how fast an object is moving.

Lorentz transform of world line
Lorentz transform of world line
Andromeda galaxy Ssc2005-20a1
Andromeda galaxy Ssc2005-20a1

There are even theoretical limits to how small a measurement of time can be. Scientists discuss a concept called Planck time. This is the smallest time step that is theoretically observable. It is approximately 5.391 × 10⁻⁴⁴ seconds. This number is much smaller than anything our current clocks can measure. On a much larger scale, scientists look at the beginning of time itself. According to the Big Bang theory, time began with the universe about 13.8 billion years ago. This connects the tiny measurements of atomic clocks to the massive history of the entire cosmos.

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🖼️ Images & Media (5)
File:Pendule de Foucault.jpg
Pendule de Foucault.jpg
File:Andromeda galaxy Ssc2005-20a1.jpg
Andromeda galaxy Ssc2005-20a1.jpg
File:Relativity of Simultaneity.svg
Relativity of Simultaneity.svg
File:Lorentz transform of world line.gif
Lorentz transform of world line.gif
File:WMAP.jpg
WMAP.jpg
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