Messier 5 (NGC 5904): A Glorious Globular and Summertime Rose

Messier 5, also referred to as the Rose Cluster, is a globular cluster in the constellation Serpens. It’s best viewed in summer.

On the night of May 5, 1702, Gottfried Kirch was comet hunting with his wife Maria when they discovered a “nebulous star” in the constellation of Serpens. The Kirches stumbled upon one of the largest, brightest, and oldest clusters in the heavens — a cluster measuring 165 light-years across!

Messier 5 (M5) is a popular target for backyard astronomers. Where else can you stare directly into 100,000 stars at once? So, the next summer night you’re star-hopping, be sure to navigate your way to one of the greatest clusters in the sky. On a clear, dark night, you can find the cluster with the naked eye. With binoculars, it looks like a fuzzy patch.

My Observations

DateJune 25, 2020
Time11:15 pm
LocationSeattle, WA
Magnification169x
ScopeMeade 8″ SCT
Eyepiece12mm
SeeingAverage
TransparencyAverage
Sketch of the globular cluster Messier 5 in the constellation Serpens as viewed through an 8-inch SCT scope and a 12mm eyepiece. The drawing shows what M5 looks like under light polluted skies. Also known as NGC 5904.
Sketch of Messier 5

June 25, 2020, at 11:15 p.m. observation: Messier 5 lives up to its reputation as a beautiful and engaging sky object. The center is bright and dense. The longer I stare into the eyepiece, more individual stars pop out of varying brightness as if I’m seeing Christmas tree lights from afar. A great target even under suburban skies.

June 5, 2023, at 10:50 pm PDT: On this evening before I pack up, I’ve decided to return to M5 to resketch it. My original drawing from 2020 never came out well. I forgot how nice and bright this globular is. And, my observation from 2020 is still true regarding how stars seem to pop out as I stare at the cluster longer.

Key Stats

ConstellationSerpens
Best ViewingSummer
Visual Magnitude+5.7
Absolute Magnitude-8.7
Distance from Earth24,000 ly
Diameter165 ly
Apparent Size23 arcmin
Milky Way LocationOrion Arm
My Viewing GradeB

Historical Observations

May 23 and 24, 1764 observation by Charles Messier

“The night of May 23 to 24, 1764, I have discovered a beautiful nebula in the constellation of Serpens, near the star of sixth magnitude; the fifth according to the catalog of Flamsteed. That nebula doesn’t contain any star; it is round, & could have a diameter of 3 arc minutes; one can see it very well, under a good sky, with an ordinary [non-achromatic] refractor of one foot. On March 11, 1769, at about four o’clock in the morning, I have reviewed that nebula with a good Gregorian telescope of 30 pouces, which magnified 104 times, & I have ensured that it doesn’t contain any star.”

William Herschel in 1791

“With a magnifying power of 250, it is all resolved into stars: they are very close, and the appearance is beautiful. With 600, perfectly resolved. There is a considerable star not far from the middle; another not far from one side, but out of the cluster; another pretty bright one; a great number of small ones. Here we have a case where the penetrating power of 20 fell short, when 29 resolved the nebula completely. This object requires also great magnifying power to shew the stars of it well; but that power had before been tried, in the 7-feet, as far as 460, without success, and could only give an indication of its being composed of stars; whereas the lower magnifying power of 250, with a greater penetrating power, in the 10-feet instrument, resolved the whole nebula into stars. I counted about 200 of them. The middle of it is so compressed that it is impossible to distinguish the stars.”

Sources and Notes

  • The photo of M5 on this page is provided by ESA/Hubble & NASA and is in the public domain.
  • The observation by Charles Messier is from the website: Messier.seds.org
  • The observation by William Hershel is from the website: universetoday.com
  • Sketch by Wayne McGraw

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