Hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  M 3  ·  NGC 5251  ·  NGC 5263  ·  NGC 5272
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M3, 



    
        

            Joey Troy
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M3

Getting plate-solving status, please wait...
M3, 



    
        

            Joey Troy
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M3

Technical card

Imaging telescopes or lenses: William Optics Redcat 51

Imaging cameras: ZWO ASI533MC Pro

Mounts: Sky-Watcher EQM 35 Pro

Guiding telescopes or lenses: ZWO 30mm f/4 Mini Guide Scope

Guiding cameras: ZWO ASI 120 Mini Mono

Software: Pixinsight

Accessory: ZWO ASI Air Pro  ·  ZWO EAF Electronic Auto Focuser


Dates:April 16, 2021April 18, 2021

Frames: 32x180" (1h 36') (gain: 101.00) -10C

Integration: 1h 36'

Darks: 10

Flats: 10

Bias: 10

Avg. Moon age: 4.83 days

Avg. Moon phase: 24.61%

Bortle Dark-Sky Scale: 3.00


Astrometry.net job: 4425079

RA center: 13h 42' 13"

DEC center: +28° 22' 45"

Pixel scale: 1.572 arcsec/pixel

Orientation: 90.108 degrees

Field radius: 1.760 degrees


Resolution: 5700x5700

Data source: Backyard

Description

Messier 3 (M3 or NGC 5272) is a globular cluster of stars in the northern constellation of Canes Venatici. It was discovered on May 3, 1764,[8] and was the first Messier object to be discovered by Charles Messier himself. Messier originally mistook the object for a nebula without stars. This mistake was corrected after the stars were resolved by William Herschel around 1784.[9] Since then, it has become one of the best-studied globular clusters. Identification of the cluster's unusually large variable star population was begun in 1913 by American astronomer Solon Irving Bailey and new variable members continue to be identified up through 2004.[10]

Many amateur astronomers consider it one of the finest northern globular clusters, following only Messier 13.[1] M3 has an apparent magnitude of 6.2,[4] making it a difficult naked eye target even with dark conditions. With a moderate-sized telescope, the cluster is fully defined. It can be found by looking almost exactly halfway along the north-west line that would join Arcturus (α Boötis) to Cor Caroli (α Canum Venaticorum). Using a telescope with a 25 cm (9.8 in) aperture, the cluster has a bright core with a diameter of about 6 arcminutes and spans a total of double that.[1]

This cluster is one of the largest and brightest, and is made up of around 500,000 stars.[9] It is estimated to be 11.4 billion years old.[7] It is centered at 32,615.64 light-years (10 kpc) away from Earth.[11]

Messier 3 is quite isolated as is 31.6 kly (9.7 kpc) above the Galactic plane and roughly 38.8 kly (11.9 kpc) from the center of the Milky Way. It contains 274 known variable stars, by far the most found in any globular cluster. These include 133 RR Lyrae variables, of which about a third display the Blazhko effect of long-period modulation. The overall abundance of elements other than hydrogen and helium, what astronomers term the metallicity, is in the range of −1.34 to −1.50 dex. This value gives the logarithm of the abundance relative to the Sun; the actual proportion is 3.2–4.6% of the solar abundance. Messier 3 is the prototype for the Oosterhoff type I cluster, which is considered "metal-rich". That is, for a globular cluster, Messier 3 has a relatively high abundance of heavier elements.[12]

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M3, 



    
        

            Joey Troy