Cat's Eye Nebula Adalah
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Two color chemes HST Palette as S-IIRed H-aGreen and O-IIIBlue.
Cat's eye nebula adalah. Nebula ini ditemukan oleh William Herschel pada tanggal 15 Februari 1786. The Cats Eye nebula is a planetary nebula in the constellation Draco. It was first discovered in 1786.
Gambar yang berhasil di abadikan oleh teleskop Hubble ini tampak seperti apa yang di gambarkan oleh Alquran surat Ar-Rahman tadi. This particular planetary nebula is around 3300 light years away. The Cats Eye Nebula was formed during the death of an intermediate-sized star.
Cats eye nebula nebula mata kucing Nebula mata kucing ngc 6543 adalah nebula yang terletak sekumpulan dengan di area rasi bintang draco. NGC 6543 or The Cats Eye Nebula is a small very bright planetary nebula found in the northern constellation Draco and 3300 light-years from Earth. My image may give the false impression that it is very large however The Cats Eye is actually the bright core of a much larger complex but you really need a much larger telescope than I have to do.
Cats Eye Nebula Mawar Merah NASA Nebula Cats Eye sebelumnya adalah sebuah bintang mati yang akhirnya meledak dan menyemburkan gas yang bersinar terang seperti mawar merah. The Cats Eye is the only planetary nebula among the winding stars of the constellation Draco which lies between the Big and Little Dippers. Struktur nebula ini merupakan salah satu struktur nebula paling kompleks yang pernah diketahui.
NGC 6543 The Cats Eye Nebula A planetary nebula is an astronomical object consisting of a glowing shell of gas and plasma formed by certain types of stars at the end of their lives. A planetary nebula is the ejected shell of a red giant star at the end of a medium sized stars life. Cats Eye Nebula Nebula Mata Kucing.
In this detailed view from NASA s Hubble Space Telescope the so-called Cats Eye Nebula looks like the penetrating eye of the disembodied sorcerer Sauron from the film adaptation of The Lord of the Rings. The Cats Eye Nebula is also known as NGC6543. Eagle Nebula Nebula Elang.
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