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Spiral Galaxy M100 in Berenice's Hair - Spiral galaxy M100 in Coma Berenices - The spiral galaxy M100 is located about 60 million years ago - light from Earth. It belongs to the Virgin's galaxy cluster. Several dwarf elliptic galaxies are visible in this image, one just above M100 probably interacting. This image was obtained by Siding Spring's 3.9m telescope. In this deep image fainter galaxies appear. One seems to be involved with the faint outskirts of the large spiral. The somewhat distorted shape of the dwarf galaxy suggests it could be both influencing and being influenced by M100, and may be the cause of the asymmetry in the spiral arms. Nearby is an even fainter, elongated dwarf galaxy and elsewhere in the picture are several others, all probably members of the Virgo cluster, which spills over into the adjoining constellation of Coma Berenices

Spiral Galaxy M100 in Berenice's Hair - Spiral galaxy M100 in Coma Berenices - The spiral galaxy M100 is located about 60 million years ago - light from Earth. It belongs to the Virgin's galaxy cluster. Several dwarf elliptic galaxies are visible in this image, one just above M100 probably interacting. This image was obtained by Siding Spring's 3.9m telescope. In this deep image fainter galaxies appear. One seems to be involved with the faint outskirts of the large spiral. The somewhat distorted shape of the dwarf galaxy suggests it could be both influencing and being influenced by M100, and may be the cause of the asymmetry in the spiral arms. Nearby is an even fainter, elongated dwarf galaxy and elsewhere in the picture are several others, all probably members of the Virgo cluster, which spills over into the adjoining constellation of Coma Berenices

PIX4611307

Spiral galaxy M100 in Berenice's Hair - Spiral galaxy M100 in Coma Berenices - The spiral galaxy M100 (NGC 4321) is located about 60 million years ago - light from Earth. It belongs to the Virgin's galaxy cluster. Several dwarf elliptic galaxies are visible in this image, one just above M100 probably interacting. This face - on spiral M100, is one of the finest spirals in the Virgo galaxy cluster. As might be expected in a galaxy - rich environment, the lack of perfect symmetry in its brightest spiral arms suggests that M100 has been disturbed by gravitational interaction with its neighbours. At the top of the image is a less spectacular galaxy, a so - called 'nucleated dwarf' elliptical galaxy, probably interacting with M100

Spiral galaxy M100 in Berenice's Hair - Spiral galaxy M100 in Coma Berenices - The spiral galaxy M100 (NGC 4321) is located about 60 million years ago - light from Earth. It belongs to the Virgin's galaxy cluster. Several dwarf elliptic galaxies are visible in this image, one just above M100 probably interacting. This face - on spiral M100, is one of the finest spirals in the Virgo galaxy cluster. As might be expected in a galaxy - rich environment, the lack of perfect symmetry in its brightest spiral arms suggests that M100 has been disturbed by gravitational interaction with its neighbours. At the top of the image is a less spectacular galaxy, a so - called 'nucleated dwarf' elliptical galaxy, probably interacting with M100

Jim Misti

PIX4611305

Spiral galaxy M100 in Berenice's Hair - Spiral galaxy M100 in Coma Berenices - The spiral galaxy M100 (NGC 4321) is located about 60 million years ago - light from Earth. It belongs to the Virgin's galaxy cluster. Several dwarf elliptic galaxies are visible in this image, one just above M100 probably interacting. This face - on spiral M100, is one of the finest spirals in the Virgo galaxy cluster. As might be expected in a galaxy - rich environment, the lack of perfect symmetry in its brightest spiral arms suggests that M100 has been disturbed by gravitational interaction with its neighbours. At the top of the image is a less spectacular galaxy, a so - called 'nucleated dwarf' elliptical galaxy, probably interacting with M100

Spiral galaxy M100 in Berenice's Hair - Spiral galaxy M100 in Coma Berenices - The spiral galaxy M100 (NGC 4321) is located about 60 million years ago - light from Earth. It belongs to the Virgin's galaxy cluster. Several dwarf elliptic galaxies are visible in this image, one just above M100 probably interacting. This face - on spiral M100, is one of the finest spirals in the Virgo galaxy cluster. As might be expected in a galaxy - rich environment, the lack of perfect symmetry in its brightest spiral arms suggests that M100 has been disturbed by gravitational interaction with its neighbours. At the top of the image is a less spectacular galaxy, a so - called 'nucleated dwarf' elliptical galaxy, probably interacting with M100

Adam Block

PIX4611275

Spiral galaxy M100 in Berenice's Hair - Spiral galaxy M100 in Coma Berenices - The spiral galaxy M100 (NGC 4321) is located about 60 million years ago - light from Earth. It belongs to the Virgin's galaxy cluster. Above the galaxy a dwarf elliptical galaxy, probably interacting with M100. This image was obtained by Siding Spring's 3.9m telescope. This dominant galaxy is the face - on spiral M100, one of the finest spirals in the Virgo cluster. As might be expected in a galaxy - rich environment, the lack of perfect symmetry in its brightest spiral arms suggests that M100 has been disturbed by gravitational interaction with its neighbours. At the top of the image is the first colour picture of a much less spectacular galaxy, a so - called 'nucleated dwarf' elliptical galaxy, probably interacting with M100. Dwarf galaxies are by far the commonest kind in rich clusters such as this, but nucleated examples are quite rare

Spiral galaxy M100 in Berenice's Hair - Spiral galaxy M100 in Coma Berenices - The spiral galaxy M100 (NGC 4321) is located about 60 million years ago - light from Earth. It belongs to the Virgin's galaxy cluster. Above the galaxy a dwarf elliptical galaxy, probably interacting with M100. This image was obtained by Siding Spring's 3.9m telescope. This dominant galaxy is the face - on spiral M100, one of the finest spirals in the Virgo cluster. As might be expected in a galaxy - rich environment, the lack of perfect symmetry in its brightest spiral arms suggests that M100 has been disturbed by gravitational interaction with its neighbours. At the top of the image is the first colour picture of a much less spectacular galaxy, a so - called 'nucleated dwarf' elliptical galaxy, probably interacting with M100. Dwarf galaxies are by far the commonest kind in rich clusters such as this, but nucleated examples are quite rare

PIX4611342

Spiral galaxy NGC 5248 in Bovier - Spiral galaxy NGC 5248 in Botes - NGC 5248 is a spiral galaxy located about 50 million years ago - light. It belongs to the Virgin's galaxy cluster. NGC 5248 is a spiral galaxy that is part of the Virgo Cluster: however on a star chart the galaxy is found to be within constellation boundaries of Bootes. Short exposures of this galaxy show the bright structures of the central regions. Many dust lanes, HII (red) regions, and blue stellar associations populate this busy area. Deeper exposures such as the image to the left begin to show the two tenous and dim outer arms of the galaxy. This galaxy seems to be a mix between M81 with two distinct arms and M100 with detailed nucleus. NGC 5248 is estimated to be 50 million light years away

Spiral galaxy NGC 5248 in Bovier - Spiral galaxy NGC 5248 in Botes - NGC 5248 is a spiral galaxy located about 50 million years ago - light. It belongs to the Virgin's galaxy cluster. NGC 5248 is a spiral galaxy that is part of the Virgo Cluster: however on a star chart the galaxy is found to be within constellation boundaries of Bootes. Short exposures of this galaxy show the bright structures of the central regions. Many dust lanes, HII (red) regions, and blue stellar associations populate this busy area. Deeper exposures such as the image to the left begin to show the two tenous and dim outer arms of the galaxy. This galaxy seems to be a mix between M81 with two distinct arms and M100 with detailed nucleus. NGC 5248 is estimated to be 50 million light years away

Adam Block

PIX4612561

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