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Newton's First Law: Introduction01:17

Newton's First Law: Introduction

Motion draws our attention. Motion itself can be beautiful, causing us to marvel at the forces needed to create spectacular sights, such as that of a dolphin jumping out of the water, the flight of a bird, or the orbit of a satellite. The study of motion is kinematics, but kinematics only describes the way objects move—their velocity and acceleration. Dynamics considers the forces that affect the motion of moving objects and systems. Newton's laws of motion are the foundation of dynamics. These...
Gravitation01:16

Gravitation

In the years before Newton, a general belief prevailed that different laws governed objects in the sky than objects on Earth. When Kepler wrote down the three laws of planetary motion, explaining in detail the geometrical properties of the planetary orbits around the Sun, there was no immediate idea to discern their connection with more fundamental laws. It was Isaac Newton who, in 1665–66, figured out the connection between planetary motion, the motion of the moon around the Earth, and the...
Space-Time Curvature and the General Theory of Relativity01:17

Space-Time Curvature and the General Theory of Relativity

In 1905, Albert Einstein published his special theory of relativity. According to this theory, no matter in the universe can attain a speed greater than the speed of light in a vacuum, which thus serves as the speed limit of the universe.
This has been verified in many experiments. However, space and time are no longer absolute. Two observers moving relative to one another do not agree on the length of objects or the passage of time. The mechanics of objects based on Newton's laws of motion,...
Influence of Earth's Curvature and Atmospheric Refraction on Leveling01:26

Influence of Earth's Curvature and Atmospheric Refraction on Leveling

During leveling, the Earth's curvature and atmospheric refraction introduce deviations in the line of sight from a true horizontal reference. When the line of sight is leveled, it remains perpendicular to the plumb line only at a single point. Beyond this, it deviates due to the Earth’s curvature, represented by the correction C. For a sight distance D, the deviation can be derived using the relationship:This relationship shows that the deviation increases quadratically with distance. Over a...
Newton's Second Law00:55

Newton's Second Law

Newton's second law is closely related to his first law of motion. It mathematically gives the cause-and-effect relationship between force and changes in motion. Newton's second law is quantitative and is used extensively to calculate what happens in situations involving a force. All external forces acting on a system add together to produce a net force Fnet. A larger net external force produces a larger acceleration. This acceleration is directly proportional to, and in the same direction as,...
Interference and Diffraction02:18

Interference and Diffraction

Interference is a characteristic phenomenon exhibited by waves. When two electromagnetic waves interact with their peaks and troughs coinciding, a resulting wave with enhanced amplitude is produced. This is known as constructive interference. In this case, the two waves interacting are in phase with each other.

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Related Experiment Video

Updated: Jun 27, 2026

Bringing the Visible Universe into Focus with Robo-AO
10:35

Bringing the Visible Universe into Focus with Robo-AO

Published on: February 12, 2013

Isaac Newton and the astronomical refraction.

Waldemar H Lehn1

  • 1Department of Electrical and Computer Engineering, University of Manitoba, Winnipeg R3T 5V6, Canada. lehn@ee.umanitoba.ca

Applied Optics
|November 28, 2008
PubMed
Summary

Isaac Newton developed two mathematical models for astronomical refraction in 1694. Researchers have now identified the exact equations he used, confirming his pioneering work in the field.

Area of Science:

  • Physics
  • Astronomy
  • Mathematical Modeling

Background:

  • Isaac Newton developed theories on astronomical refraction in 1694 but did not publish them.
  • Previous research since 1836 has attempted to reconstruct Newton's methods and equations for astronomical refraction.
  • Identifying Newton's original mathematical models and calculations for atmospheric refraction remains a historical challenge.

Purpose of the Study:

  • To identify the specific mathematical models and equations Isaac Newton used for astronomical refraction.
  • To reconstruct and verify Newton's calculations for astronomical refraction tables.
  • To establish Newton as the first to derive accurate equations for astronomical refraction.

Main Methods:

  • A closed-form solution was identified for the refraction integral of Newton's first model, which assumes a linear density decay with elevation.

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Last Updated: Jun 27, 2026

Bringing the Visible Universe into Focus with Robo-AO
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Published on: February 12, 2013

In Situ Measurement of Vacuum Window Birefringence using 25Mg+ Fluorescence
07:03

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  • Newton's second model, incorporating exponential atmospheric pressure variation, was analyzed by reproducing its results.
  • The identified solutions and parameters were compared against Newton's calculated refraction tables.
  • Main Results:

    • A closed-form solution was found that accurately reproduces the refraction table for Newton's first model.
    • The parameters for Newton's second model were successfully identified by replicating his results.
    • Both identified models and equations precisely match Newton's original calculations.

    Conclusions:

    • Isaac Newton derived the correct equations for astronomical refraction for both of his models.
    • Newton's work predates and surpasses previous attempts to model astronomical refraction.
    • This study confirms Newton's foundational contributions to the understanding of astronomical refraction.