Spiral galaxy in the constellation Pegasus (NGC 7217)

Name in the directory:NGC_7217
Category:Galaxy
Right Ascension:22h 8m 1.92s
Declination:+31° 16′ 55.56″
Total Exposure:8 часов 39 минут
Number of Frames:173
Link to FITS files:Download
  • L141 minutes (47 frames)
  • G123 minutes (41 frames)
  • R126 minutes (42 frames)
  • B129 minutes (43 frames)

NGC 7217 is a spiral galaxy located in the constellation Pegasus. It is notable for its multiple concentric rings of stars and dust.

Features

One of the unique features of the galaxy is a group of stars in the core that move in different directions, which attracts the attention of astronomers. These stars also vary in age, which may indicate a complex history of its formation.

Galaxy merger

NGC 7217 is believed to be the result of a merger of two disk galaxies, each of which was rotating in opposite directions. Computer simulations support the hypothesis that the purple galaxy swallowed a smaller spiral galaxy, rich in gas. This process led to a burst of star formation.

NGC 4550

At the center of NGC 7217 is the galaxy NGC 4550, which contains small amounts of molecular hydrogen and interstellar dust.

PhotoDateFramesExposureLRGB
24 Apr 202217311:3203:0802:4802:4402:52
24 Aug 202116811:1202:4802:4802:4402:52

Visibility chart of Spiral galaxy in the constellation Pegasus (NGC 7217) during the day

The height diagram of Spiral galaxy in the constellation Pegasus (NGC 7217) above the horizon during the current day for the observatory observation point in Orenburg (51.7, 55.2). The chart shows when the object is above the horizon and at what maximum height in degrees it rises. The data is relevant for the observation date: Saturday, 26 April 2025.
DateMoon PhaseExposureCCD TemperatureGainOffsetFilter
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