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how is luminosity class assigned to a star

by Prof. Emmalee Bartell IV Published 3 years ago Updated 2 years ago

How is a luminosity class assigned to a star? By studying the absorption line width in the spectrum of the star.

Full Answer

What is the luminosity class of a star?

Because this line‐width classification correlates with luminosity, the designation Ia to V is termed a luminosity class. The full spectral classification of a star therefore includes both the spectral type (OBAFGKM) as well as its luminosity class (I‐V); for example, we would classify the Sun as a G2 V star.

What are the different types of luminosity classifications?

Luminosity Classes. Type V stars are like the Sun, dwarf or Main Sequence stars, which are fainter than the larger stars. Because this line‐width classification correlates with luminosity, the designation Ia to V is termed a luminosity class. The full spectral classification of a star therefore includes both the spectral type (OBAFGKM)...

Is type V a luminosity class?

Type V stars are like the Sun, dwarf or Main Sequence stars, which are fainter than the larger stars. Because this line‐width classification correlates with luminosity, the designation Ia to V is termed a luminosity class.

What is the full spectral classification of a star?

The full spectral classification of a star therefore includes both the spectral type (OBAFGKM) as well as its luminosity class (I‐V); for example, we would classify the Sun as a G2 V star.

How do you determine the luminosity class of a star?

Luminosity classes are labeled with Roman numerals from I to V: I are supergiant stars, II are bright giants, III are ordinary giants, IV are subgiants, and V are ordinary main sequence stars.

What is luminosity classification?

A classification of stars according to their luminosity, which can vary widely for a given spectral type. Luminosity class indicates, for example, whether a star is a supergiant, a giant, or a dwarf.

What determines the luminosity of a main-sequence star?

The luminosity and temperature of a main-sequence star are set by its mass. More massive means brighter and hotter. A ten solar mass star has about ten times the sun's supply of nuclear energy. Its luminosity is 3000 times that of the sun.

HOW IS A stars spectral class determined?

The spectral types and sub-classes represent a temperature sequence, from hotter (O stars) to cooler (M stars), and from hotter (subclass 0) to cooler (subclass 9). The temperature defines the star's "color" and surface brightness.

What is luminosity of a star?

Astronomers also measure luminosity — the amount of energy (light) that a star emits from its surface. Measuring star brightness is an ancient idea, but today astronomers use more precise tools to obtain the calculation.

How do you classify a star?

Astronomers classify stars according to their physical characteristics. Characteristics used to classify stars include color, temperature, size, composition, and brightness. Stars vary in their chemical composition.

How does luminosity change on main sequence?

The luminosity of a star remains approximately constant during its time on the main sequence. There is a slight increase over time, which is, as you guessed, related to the changing composition of the star due to fusion.

How is luminosity calculated?

How is luminosity calculated? In order to calculate luminosity, the mathematical constant "pi" (3.14) is used. The distance of the object from Earth in square meters is multiplied by the object's brightness in watts per square meters. That is then multiplied by 3.14 and then again by 4 to calculate luminosity.

Why does luminosity increase on the main sequence?

The greater the mass of a main sequence star, the greater its effective temperature. This, combined with the larger radius of higher mass main sequence stars accounts for their much greater luminosity. Remember, L ∝ T4 and L ∝ R2 so even a small increase in effective temperature will significantly increase luminosity.

How are spectral classes arranged?

In the MK system, a luminosity class is added to the spectral class using Roman numerals. This is based on the width of certain absorption lines in the star's spectrum, which vary with the density of the atmosphere and so distinguish giant stars from dwarfs.

What is spectral classification based on?

Stars are classified based on the properties of their spectra, primarily the absorption lines present due to metals in the outer layers of the star. These properties are determined primarily by the temperature of the star, but the physical size of the star also plays a role.

What does OH a fine girl kiss me mean?

Every student in introductory astronomy learns the mnemonic “Oh Be a Fine Girl/Guy, Kiss Me”, which is a way to remember the spectral classification of stars. Here's how it works: the color of a star is determined by its temperature, as I outlined previously.

What is Luminosity?

Professional astronomers, amateurs or anyone who has looked up in the nighttime sky has probably noticed the star Sirius. Located in the constellation Canis Major, Sirius is the brightest star visible on Earth, aside from the Sun. However, this does not mean that Sirius generates the most energy nor is the largest or hottest star.

Luminosity of a Star

The luminosity of a star has a direct correlation with its temperature. Many stars in the Milky Way use nuclear fusion to generate energy. Nuclear fusion occurs under intense pressure when the lighter nuclei of atoms combine to form heavier atoms.

Luminosity Formula

To calculate the luminosity of a star using brightness, astronomers use the formula:

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