Celsius
The Celsius scale, also known as the centigrade scale, is a temperature scale used in the metric system. It was developed by Anders Celsius in 1742. The Celsius scale is based on 0°C for the freezing point of water and 100°C for the boiling point of water at 1 atm pressure. This makes it easy to use for scientific and everyday purposes.
Conversion Formula
To convert a temperature from Celsius to Fahrenheit, you can use the formula:
Fahrenheit = (Celsius × 9/5) + 32
Study Guide
- Understand the concept of the Celsius scale and its key reference points.
- Practice converting temperatures between Celsius and Fahrenheit using the conversion formula.
- Learn about the historical background and significance of the Celsius scale in the field of temperature measurement.
- Explore real-life applications of the Celsius scale, such as weather forecasting and scientific experiments.
◂Physics Worksheets and Study Guides High School. Rotational Motion/Universal Gravitation
Worksheet/Answer key
Rotational Motion/Universal Gravitation 
Worksheet/Answer key
Rotational Motion/Universal Gravitation Worksheet/Answer key
Rotational Motion/Universal Gravitation
Worksheet/Answer keyWorksheet/Answer keyThe resources above cover the following skills:
EARTH AND SPACE SCIENCE (NGSS)
Earth’s Place in the Universe
Students who demonstrate understanding can:
Use mathematical or computational representations to predict the motion of orbiting objects in the solar system.
EARTH AND SPACE SCIENCE (NGSS)
Earth’s Place in the Universe
Students who demonstrate understanding can:
Use mathematical or computational representations to predict the motion of orbiting objects in the solar system.
EARTH AND SPACE SCIENCE (NGSS)
Earth’s Place in the Universe
Students who demonstrate understanding can:
Use mathematical or computational representations to predict the motion of orbiting objects in the solar system.
EARTH AND SPACE SCIENCE (NGSS)
Earth’s Place in the Universe
Students who demonstrate understanding can:
Use mathematical or computational representations to predict the motion of orbiting objects in the solar system.