Spiral galaxies are stunning, swirling collections of stars, gas, and dust with arms that create new stars, first described by Edwin Hubble in 1936.
Overview
Famous Spiral Galaxies
Formation And Evolution
The Role Of Dark Matter
Observational Techniques
Structure And Components
Spiral Arms And Star Formation
Current Research And Discoveries
The Milky Way As A Spiral Galaxy
Characteristics Of Spiral Galaxies
Comparison With Other Galaxy Types
Hubble Space Telescope
Gravitational Lensing
Triangulum Galaxy
Andromeda Galaxy
Edwin Hubble
Dark Matter
Sagittarius
Technology
Building
Gravity
Oval
๐ Spiral galaxies look like giant swirling pinwheels made up of stars, gas, and dust.
๐ Our home galaxy, the Milky Way, is a spiral galaxy!
๐ Spiral galaxies can have tight or loose arms, depending on how they are wound.
๐ The arms of spiral galaxies are where most new stars are born!
๐ Spiral galaxies are surrounded by a halo of dark matter that we can't see.
๐ซ The Andromeda Galaxy is the closest spiral galaxy to the Milky Way, about 2.537 million light-years away!
๐ญ Astronomers use telescopes to capture images and study spiral galaxies in different types of light.
๐ The arms of spiral galaxies often have hot, young stars that create colorful light!
๐ The Milky Way has approximately four main spiral arms named Perseus, Sagittarius, Scutum-Centaurus, and Norma.
๐ Dark matter plays a crucial role in holding spiral galaxies together and influencing their rotation.
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