Location settings
GPS
37.8°/-97.8°
GMT -6
Waning18:58 - 06:31
🔎
☰
Sky-Tonight.com / Nebulae / NGC2420

NGC2420 Observation Details

NGC2420

NGC2420 Daily Motion

NGC2420 will rise at 15:53, reaching 35° when twilight begins at 18:58. It will reach transit at 74° by 23:03 and will set before twilight ends at 06:13.
NGC2420 will be visible until May, 22, when it will move too close to the Sun. During this time, its proximity to the Sun will cause it to disappear from the night sky, making it unobservable for a while.

NGC2420 Visibility Timetable on February 06

Rise and Set Timetable

TimeElevation
Moon Rise, 54.6% illuminated11:27-30°
NGC2420 rise15:53
Sunset17:5823°
Civil sunset18:2729°
Astrosession begin19:2941°
NGC2420 transit23:0374°
Moon Set02:4041°
Astrosession end06:012°
NGC2420 set06:13

Track NGC2420 Position Throughout the Night

← Thu, 6 February 2025 →

Elevation (degrees)
Time
Altitude
Azimuth
Shift the map to change the time and observe NGC2420 changing position in the night sky.

NGC2420 Image Gallery

DSS Blue

NGC2420 photo taken with blue filter
These images are valuable for highlighting the presence of younger, hotter stars, which emit more light in the blue wavelengths.

DSS Red

NGC2420 photo taken with red filter
These images are excellent for detecting older, cooler stars, as well as emission nebulae, which glow primarily in the red due to hydrogen alpha emissions.

DSS Near-Infrared

NGC2420 photo taken with Near-Infrared filter
These images can penetrate dust clouds that obscure visible light, revealing structures and objects hidden within.

DSS Composite image

NGC2420 color image
DSS Color images are composite images created by combining the blue, red, and often near-infrared images to produce a full-color representation.

The photos are taken from the Digitized Sky Survey 2 (DSS2), which was produced at the Space Telescope Science Institute (STScI) under NASA contract, using data from the UK Science and Technology Facilities Council (STFC), the European Southern Observatory (ESO), and the National Geographic Society-Palomar Observatory Sky Survey (POSS II).

Special thanks to the National Optical Astronomy Observatory (NOAO), the Royal Observatory, Edinburgh, and the California Institute of Technology for their significant contributions.

Finder Chart for NGC2420

Double-click to unlock the map.
Object nameNGC2420
Field of view
Limiting magnitude
NGC2420 coordinates7.63997, 21.57408
Center coordinates7.63997, 21.57408

NGC2420 Passage Through Night

Double-click to unlock the map.

Current position of NGC2420

Time06:58
Latitude37.751
Longitude-97.822
NGC2420 elevation-7°
NGC2420 Azimuth56°
Here you can see the current position of the NGC2420 on the map, as well as its positions for rise and set. This tool allows you to track the NGC2420's movement throughout the night, providing you with accurate and up-to-date information.

Annual motion of NGC2420

Time
DateThu, 6 February 2025
Twighlight start19:24
Twighlight end05:55
Twighlight duration11h 31m
Rise15:53
Set06:13
Elevation at transit74°
Transit time23:03
Equatorial coordinateRA: 07h 38m 23s", Dec: 21° 34' 26s
Magnitude8
ConstellationGemini
The graph illustrates the annual visibility pattern of a NGC2420, providing a comprehensive overview of its daily appearances and transit times throughout the year.
The graph is structured with the vertical axis showing the hours of the day, ranging from 12 AM to 12 AM the next day, while the horizontal axis spans each day of the year.
The reddish shaded area indicates the periods when the NGC2420 is above the horizon, visible to observers. The white line marks the times when the celestial object reaches its highest point in the sky each day, known as the transit.

Data Credits

The nebulae information on this page is sourced from the OpenNGC project, developed by Matteo Verga. OpenNGC provides detailed data on the NGC catalog, which is a valuable resource for exploring deep-sky objects such as nebulae.

For more details or to contribute to OpenNGC, visit the official GitHub repository: OpenNGC on GitHub.