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Bilder zu 'Ic 1848' gefunden, 10

Nebulae IC1805 & IC1848 in Cassiopee - IC 1805, IC 1848, The Double Nebula 300 mm f/2.8 ED Nikkor lens Composite of two 20 minute exposures Lumicon Deep Sky Filter hypered Kodak Pro 400 PPF 1:37 and 2:00 am September 20, 1996 Chatsworth, N

Nebulae IC1805 & IC1848 in Cassiopee - IC 1805, IC 1848, The Double Nebula 300 mm f/2.8 ED Nikkor lens Composite of two 20 minute exposures Lumicon Deep Sky Filter hypered Kodak Pro 400 PPF 1:37 and 2:00 am September 20, 1996 Chatsworth, N

Jerry Lodriguss

PIX4622322

Detail in the nebula IC 1848 in Cassiopee - Close up of IC 1848 in Cassiopeia - Detail in the northern part of the nebula. IC 1848 close up in the northern portion of the nebula

Detail in the nebula IC 1848 in Cassiopee - Close up of IC 1848 in Cassiopeia - Detail in the northern part of the nebula. IC 1848 close up in the northern portion of the nebula

Adam Block

PIX4622403

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

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

Detail in nebula IC 1848 in Cassiopee - Detail in nebula IC 1848 in Cassiope

Detail in nebula IC 1848 in Cassiopee - Detail in nebula IC 1848 in Cassiope

PIX4622449

Constellation of Taurus - Constellation of Taurus - On the right of the image, nebula NGC 1499, on the top, nebulae IC 1805 and IC 1848

Constellation of Taurus - Constellation of Taurus - On the right of the image, nebula NGC 1499, on the top, nebulae IC 1805 and IC 1848

B&S.Fletcher

PIX4594054

Persee Constellation - Constellation of Perseus - At the top of the picture, nebulae IC 1805 - 1848, the double cluster of Persee, bottom nebula NGC 1499

Persee Constellation - Constellation of Perseus - At the top of the picture, nebulae IC 1805 - 1848, the double cluster of Persee, bottom nebula NGC 1499

B&S.Fletcher

PIX4593194

This WISE mosaic is of the Soul Nebula (a.k.a. the Embryo Nebula, IC 1848, or W5). It is an open cluster of stars surrounded by a cloud of dust and gas over 150 light-years across and located about 6,500 light-years from Earth in the constellation Cassiopeia, near the Heart Nebula.

This WISE mosaic is of the Soul Nebula (a.k.a. the Embryo Nebula, IC 1848, or W5). It is an open cluster of stars surrounded by a cloud of dust and gas over 150 light-years across and located about 6,500 light-years from Earth in the constellation Cassiopeia, near the Heart Nebula.

UIG867150

This WISE mosaic is of the Soul Nebula (a.k.a. the Embryo Nebula, IC 1848, or W5). It is an open cluster of stars surrounded by a cloud of dust and gas over 150 light-years across and located about 6,500 light-years from Earth in the constellation Cassiopeia, near the Heart Nebula.

This WISE mosaic is of the Soul Nebula (a.k.a. the Embryo Nebula, IC 1848, or W5). It is an open cluster of stars surrounded by a cloud of dust and gas over 150 light-years across and located about 6,500 light-years from Earth in the constellation Cassiopeia, near the Heart Nebula.

UIG867151

Nebulae IC 1848 and IC 1805 in Cassiopee - The north is at top. IC1848 nebula and the star cluster embedded in it are located just 4 degrees north of h Persei, one of the two members of the famous Double Cluster. The same nebula also hosts Collinder 33 (Cr33) and Collinder 34 (Cr34) star clusters. The faint nebulae IC1871 and Sh2 - 198 are just near the IC1848. Just one and a half degree north - west from IC1848 is located the IC1805 complex. This rich but faint nebular complex resides 5* NNE of the Double Cluster in Perseus. The largest and very diffuse part of it, IC1805, contains large and bright star cluster Melotte 15 at its center. Other star clusters (NGC1027, Berkeley 65 and Markarian 6) are located around its edges. The brightest part of IC1805 complex consists of nebulae IC1795 and NGC896 which together are intersected by narrow NW to SE streaks of dust. Also the two Maffei galaxies are included in this view at bottom center. This image is based on data acquired by the Oschin

Nebulae IC 1848 and IC 1805 in Cassiopee - The north is at top. IC1848 nebula and the star cluster embedded in it are located just 4 degrees north of h Persei, one of the two members of the famous Double Cluster. The same nebula also hosts Collinder 33 (Cr33) and Collinder 34 (Cr34) star clusters. The faint nebulae IC1871 and Sh2 - 198 are just near the IC1848. Just one and a half degree north - west from IC1848 is located the IC1805 complex. This rich but faint nebular complex resides 5* NNE of the Double Cluster in Perseus. The largest and very diffuse part of it, IC1805, contains large and bright star cluster Melotte 15 at its center. Other star clusters (NGC1027, Berkeley 65 and Markarian 6) are located around its edges. The brightest part of IC1805 complex consists of nebulae IC1795 and NGC896 which together are intersected by narrow NW to SE streaks of dust. Also the two Maffei galaxies are included in this view at bottom center. This image is based on data acquired by the Oschin

D. De Martin

PIX4622341

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