The temperature of the Sun is approximately 6000 °C. What is this in Fahrenheit?

The Sun is the closest star to Earth and the primary source of heat and light for our planet. Its surface temperature is about 6000 °C, which is extremely hot compared to temperatures experienced on Earth. To understand this temperature in the Fahrenheit scale, the standard conversion formula is applied:

$$°F=(°C\times 9/5)+32$$

Applying it to 6000 °C:

$$°F=(6000\times 9/5)+32°F=10800+32°F=10,832$$

Hence, the Sun’s surface temperature is approximately 10,832 °F.

Understanding the Sun’s temperature is important in astronomy, physics, and everyday science:

1. 
   

   Solar radiation: The Sun emits energy in the form of light and heat, which sustains life on Earth.

   
   


2. 
   

   Astronomical studies: Knowledge of the Sun’s temperature helps scientists classify stars, understand nuclear fusion, and predict solar activity.

   
   


3. 
   

   Practical conversions: Students and professionals often need to convert temperatures between Celsius, Fahrenheit, and Kelvin for experiments and calculations.

   
   

Comparison with the options:

• 
  

  8000 °F → too low

  
  


• 
  

  9000 °F → slightly low

  
  


• 
  

  10,832 °F → correct

  
  


• 
  

  None of these → incorrect

  
  

By converting 6000 °C to Fahrenheit, students gain practical skills in unit conversion and a better understanding of extreme temperatures in the universe.

Thus, the Sun’s temperature in Fahrenheit is approximately 10,832 °F (Option C).