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Cygnus as depicted in Urania's Mirror, a set of constellation cards published in London c.1825. Surrounding it are Lacerta, Vulpecula and Lyra.
Cygnus as depicted in Urania's Mirror, a set of constellation cards published in London c.1825. Surrounding it are Lacerta, Vulpecula and Lyra.
Cygnus is superimposed as main stars constellation over a photo of the according section of the night sky
Cygnus is superimposed as main stars constellation over a photo of the according section of the night sky
On the left side of this X-ray image are the bright North America Nebula (left bright part) with Sadr region (right bright part) in the Cygnus X regio
On the left side of this X-ray image are the bright North America Nebula (left bright part) with Sadr region (right bright part) in the Cygnus X region, visually interrupted by the Cygnus rift .
The constellation Cygnus as it can be seen by the naked eye, with the Northern Cross in the middle.
The constellation Cygnus as it can be seen by the naked eye, with the Northern Cross in the middle.
Lyra
The constellation Lyra as it can be seen by the naked eye.
The constellation Lyra as it can be seen by the naked eye.
The constellation Lyra, enhanced for color and contrast. Brightest five stars are labeled.
The constellation Lyra, enhanced for color and contrast. Brightest five stars are labeled.
A long-exposure image of Lyra
A long-exposure image of Lyra
Messier 56 is composed of a large number of stars, tightly bound to each other by gravity. In Lyra are the objects M56, M57, and Kuiper 90. M56 is a r
Messier 56 is composed of a large number of stars, tightly bound to each other by gravity. In Lyra are the objects M56, M57, and Kuiper 90. M56 is a rather loose globular cluster at a distance of approximately 32,900 light-years, with a diameter of about 85 light-years. Its apparent brightness is 8.3m.