UDF 2457
UDF 2457 is the Hubble Ultra Deep Field (UDF) identifier for a red dwarf star calculated to be about 59,000 light-years (18 kiloparsecs) from Earth with a very dim apparent magnitude of 25. The Milky Way galaxy is about 100,000 light-years in diameter, and the Sun is about 25,000 light-years from the galactic center. The small common star UDF 2457 may be one of the farthest known stars inside the main body of the Milky Way. Globular clusters (such as Messier 54 and NGC 2419) and stellar streams are located further out in the galactic halo.
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UDF 2457
UDF 2457 is the Hubble Ultra Deep Field (UDF) identifier for a red dwarf star calculated to be about 59,000 light-years (18 kiloparsecs) from Earth with a very dim apparent magnitude of 25. The Milky Way galaxy is about 100,000 light-years in diameter, and the Sun is about 25,000 light-years from the galactic center. The small common star UDF 2457 may be one of the farthest known stars inside the main body of the Milky Way. Globular clusters (such as Messier 54 and NGC 2419) and stellar streams are located further out in the galactic halo.
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UDF 2457 is the Hubble Ultra D ...... ther out in the galactic halo.
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UDF 2457とは、地球から見てろ座の方向に5万9000光 ...... 団内の恒星を除けば、最も遠い銀河系の恒星である可能性がある。
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29,389,753
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732,881,048
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Red dwarf star UDF 2457 as seen by the Hubble Ultra Deep Field
UDF 2457 is located above the ...... f the Hubble Ultra Deep Field.
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UDF 2457 is the Hubble Ultra D ...... ther out in the galactic halo.
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UDF 2457とは、地球から見てろ座の方向に5万9000光 ...... 団内の恒星を除けば、最も遠い銀河系の恒星である可能性がある。
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UDF 2457
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UDF 2457
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UDF 2457
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