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There are several schemes in use by which galaxies can be classified according to their morphologies, the most famous being the hubble sequence, devised by edwin hubble and later expanded by gérard de vaucouleurs and allan sandage. He classified spiral and barred spiral galaxies further according to the size of their central bulge and the texture of their arms. First look at classifying galaxies the image above is called hubble’s tuning fork
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It was developed by edwin hubble, who was the first person to classify galaxies based on their morphology. Spirals, barred spirals, ellipticals and irregulars As one of the first steps towards a coherent theory of galaxy evolution, the american astronomer edwin hubble, developed a classification scheme of galaxies in 1926.
Method of classifying galaxies according to their appearance, developed by edwin hubble.
The major types classified by hubble included elliptical galaxies, spiral galaxies, and barred spiral galaxies He also noted additional types such as lenticular and irregular galaxies. After he discovered what galaxies really were, edwin hubble became the first person to classify galaxies Astronomers use his system, called the “hubble tuning fork,” even today
First, hubble divided the galaxies into two general categories Edwin hubble’s tuning fork diagram divides galaxies into three groups Elliptical, spiral, and irregular galaxies Elliptical galaxies are classified by how round or flat they look.
Edwin hubble was the first to classify galaxies based on the shapes, which he observed
These observations included elliptical galaxies, spiral galaxies, and irregular galaxies. After he established the extragalactic nature of some types of nebulae, edwin hubble tried to define ways to classify these new galaxies according to their appearance, or galactic morphology. Edwin hubble invented a classification of galaxies and grouped them into four classes
