Enter the total time (hrs) and the no light time (hrs) into the Calculator. The calculator will evaluate the Light Time. 

Light Time Formula

LT = TT - NT

Variables:

  • LT is the Light Time (hrs)
  • TT is the total time (hrs)
  • NT is the no light time (hrs)

To calculate Light Time, subtract the no light time from the total time.

How to Calculate Light Time?

The following steps outline how to calculate Light Time.


  1. First, determine the total time (hrs). 
  2. Next, determine the no light time (hrs). 
  3. Next, gather the formula from above = LT = TT – NT.
  4. Finally, calculate the Light Time.
  5. After inserting the variables and calculating the result, check your answer with the calculator above.

Example Problem : 

Use the following variables as an example problem to test your knowledge.

total time (hrs) = 24

no light time (hrs) = 12

Frequently Asked Questions (FAQ)

What is Light Time in the context of physics?

Light Time refers to the duration during which an area or object receives light. In physics, it can also relate to the time taken by light to travel from one point to another in space.

How does the speed of light affect Light Time calculations?

The speed of light is a constant (approximately 299,792 kilometers per second in a vacuum), and it directly affects Light Time calculations when measuring the distance light travels over a period. However, in the context of this calculator, Light Time is calculated based on hours of exposure, not the distance light travels.

Can the Light Time formula be applied to astronomical observations?

Yes, the concept of Light Time is crucial in astronomy for calculating the time it takes for light from celestial objects to reach Earth. This helps in understanding the actual position and characteristics of stars and galaxies relative to their observed position.

Why is it important to calculate no light time in certain scenarios?

Calculating no light time is essential in various scientific and practical scenarios, such as plant growth in agriculture, where understanding periods of darkness is as critical as light exposure. It’s also important in photography (for exposure calculations) and in designing lighting systems for controlled environments.