'Lbn 667' Bilder und Clips Suchergebnisse page 1 of 1

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Nebulae IC 1805 and IC 1848 and the double cluster of Persee - The Double Cluster and Double Nebula - The double cluster of Persee (NGC 884 and NGC 869) is visible at the top left of the image. IC 1848 (upper right) is an emission nebula associated with a cluster of stars; it also houses the CR 34 star cluster. Lower right, the largest nebula, IC 1805. The Double Cluster in Perseus (NGC 884 and NGC 869) is at upper left. The Double Nebulae, at right, are two large complexes of faint emission nebulosity in Cassiopeia. LBN 667 is at upper right. IC 1805 is at lower right. Both are red hydrogen - alpha emission nebulae. The large loose open cluster Stock 2 is just below and left of center. This incredibly star - rich area of sky lies in the Milky Way on the border of Cassiopeia and Perseus

Nebulae IC 1805 and IC 1848 and the double cluster of Persee - The Double Cluster and Double Nebula - The double cluster of Persee (NGC 884 and NGC 869) is visible at the top left of the image. IC 1848 (upper right) is an emission nebula associated with a cluster of stars; it also houses the CR 34 star cluster. Lower right, the largest nebula, IC 1805. The Double Cluster in Perseus (NGC 884 and NGC 869) is at upper left. The Double Nebulae, at right, are two large complexes of faint emission nebulosity in Cassiopeia. LBN 667 is at upper right. IC 1805 is at lower right. Both are red hydrogen - alpha emission nebulae. The large loose open cluster Stock 2 is just below and left of center. This incredibly star - rich area of sky lies in the Milky Way on the border of Cassiopeia and Perseus

Jerry Lodriguss

PIX4622368

Nebulas IC 1805 and IC 1848 in Cassiopee - Nebulas IC 1805 and IC 1848 in Cassiopeia - IC 1848 (left) is an emission nebula associated with a cluster of stars; it also houses the CR 34 star cluster. On the right, the largest nebula, IC 1805. LBN 667 is the large area of red emission nebulosity on the left side of the image. Open clusters CR 34 and IC 1848 are embedded in the nebula. IC 1805 is the large area of nebulosity on the right side of the image. NGC 896, a bright knot of nebulosity, is at the upper right of the photo. IC 1805 looks vaguely like a heart if you rotate your head 90 degrees counterclockwise and use your imagination when you look at the photo. The loose open cluster Mel 15 lies at the center of IC 1805, and open cluster NGC 1027 is just above right of the center of the image at top

Nebulas IC 1805 and IC 1848 in Cassiopee - Nebulas IC 1805 and IC 1848 in Cassiopeia - IC 1848 (left) is an emission nebula associated with a cluster of stars; it also houses the CR 34 star cluster. On the right, the largest nebula, IC 1805. LBN 667 is the large area of red emission nebulosity on the left side of the image. Open clusters CR 34 and IC 1848 are embedded in the nebula. IC 1805 is the large area of nebulosity on the right side of the image. NGC 896, a bright knot of nebulosity, is at the upper right of the photo. IC 1805 looks vaguely like a heart if you rotate your head 90 degrees counterclockwise and use your imagination when you look at the photo. The loose open cluster Mel 15 lies at the center of IC 1805, and open cluster NGC 1027 is just above right of the center of the image at top

Jerry Lodriguss

PIX4622386

Constellation Cassiopee - The constellation of Cassiopeia - The constellation of Cassiopeia, the Queen, is seen in this wide - angle shot spanning a field of about 16 x 24 degrees. This bright section of the Milky Way is strewn with thousands of individual stars, star clouds, dark nebulae, red emission nebulae, and glittering star clusters. As we look at Cassiopeia, we are looking out into one of the outer arms of our own Milky Way galaxy, and away from the galaxy's center in Sagittarius. The Double Cluster in Perseus (NGC 884 and NGC 869) and the Double Nebulae (IC 1805 and LBN 667) are at upper right. NGC 281, another emission nebula, is near Schedar (Alpha Cassiopeiae). IC 59 and IC 63 are two small faint nebulae near Gamma Cassiopeia, in the center of the constellation. Another very large complex of red emission nebulae, Ced 214 and NGC 7822 lie near the center of the bottom of the frame, and open cluster NGC 7789 is to the left of Caph. Open cluster M52 and NGC 7635, the Bubble Ne

Constellation Cassiopee - The constellation of Cassiopeia - The constellation of Cassiopeia, the Queen, is seen in this wide - angle shot spanning a field of about 16 x 24 degrees. This bright section of the Milky Way is strewn with thousands of individual stars, star clouds, dark nebulae, red emission nebulae, and glittering star clusters. As we look at Cassiopeia, we are looking out into one of the outer arms of our own Milky Way galaxy, and away from the galaxy's center in Sagittarius. The Double Cluster in Perseus (NGC 884 and NGC 869) and the Double Nebulae (IC 1805 and LBN 667) are at upper right. NGC 281, another emission nebula, is near Schedar (Alpha Cassiopeiae). IC 59 and IC 63 are two small faint nebulae near Gamma Cassiopeia, in the center of the constellation. Another very large complex of red emission nebulae, Ced 214 and NGC 7822 lie near the center of the bottom of the frame, and open cluster NGC 7789 is to the left of Caph. Open cluster M52 and NGC 7635, the Bubble Ne

Jerry Lodriguss

PIX4589634

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