**What is Absolute Magnitude?**

It is the brightness of a celestial body viewed from a fixed distance of 10 parsecs measured in absolute magnitude (equivalent to thirty times the distance traveled by light in a year). Absolute magnitude refers to the intensity of light emitted by celestial bodies, and this tells us that its absolute magnitude drops when an object’s brightness increases. It is represented by the symbol Mv.

The absolute magnitude of a quantity can be calculated using the formula below.

2.25log([d/10]2)

Where;

d is the parsec distance.

M is the apparent magnitude.

The bolometer is used to measure the absolute magnitude, and it is a gadget that measures electromagnetic radiation.

Absolute magnitude describes the object’s intrinsic brightness, and this system ignores the energy absorbed by matter in space while measuring it. Absolute magnitude depicts the celestial body’s actual luminosity.

**What is Apparent Magnitude?**

An object’s apparent magnitude measures how bright it seems from the observer’s point of view, such as the Earth. It accounts for all the possible obstacles and absorbers of light in its route.

The symbol for apparent magnitude is mv. A reverse logarithmic scale is used for apparent magnitude. The naked eye can view celestial objects with apparent magnitudes ranging from -1 to 6.5. The apparent magnitude can be used to calculate the absolute importance as well. The formula for determining the relationship between absolute magnitude (Mv) and apparent magnitude (mv) is below.

Mathematically speaking, the difference between Mv and Mv is five log10 (d)

**Difference Between Absolute and Apparent Magnitude**

- The absolute magnitude of a celestial body is a technique of determining the intrinsic brightness of that body. The apparent magnitude of a light source is defined as the magnitude of the intelligence about the distance between the point of observation and the light source.
- It is possible to express the absolute magnitude of a celestial body’s brightness at a distance of ten parsecs from it as the object’s apparent magnitude when measuring the luminosity of a celestial body. Earth is our starting point for discussing the obvious immensity of the universe.
- The absolute magnitude does not consider any factors that may hinder the path of light emitted by the object. It refers to the actual luminance of the celestial body observed. However, apparent magnitude is determined by considering all of the variables that could influence the intensity of the light detected from the body.
- Mv denotes the absolute magnitude, but the apparent magnitude is represented by mv. The apparent magnitude is indicated by mv.
- An apparent magnitude measurement system uses photometric equipment; an absolute magnitude measurement system uses bolometers.

**Comparison Between Absolute and Apparent Magnitude**

Parameter of Comparison | Absolute Magnitude | Apparent Magnitude |

Meaning | It provides the magnitude of the brightness of a celestial body when observed from a certain distance in the night sky. | This parameter indicates the brightness of a celestial body about the observer’s location (The Earth). |

Scale used | The scale is inverse logarithmic. | The scale is in reverse logarithmic notation. |

Symbol | Mv is the symbol used to represent it. | The sign mv denotes it in this case. |

Factors on which it depends | The energy emitted by a star or a celestial body in one second. | The size of the celestial body, the quantity of energy emitted by the body, and the distance between the celestial body and the Earth are all factors to consider. |

Highlights | There is no consideration for energy wasted due to light being absorbed by cosmic dust when evaluating brightness. | When calculating the brightness, it considers all of the variables, such as the amount of energy absorbed by the interstellar material. |