Even with the best of viewing conditions, the globular star cluster Messier 5 – aka M5 – is barely detectable to the unaided eye as a faint star. In binoculars, it appears as a faint, fuzzy star. Ah, but point a small telescope its way! Some amateur observers swear that M5 is the finest globular cluster north of the celestial equator for small telescopes – even better than the celebrated M13, the Great Hercules cluster. Follow the links below to learn more about this wonderful cluster.
What is M5? Many of the brighter and larger clusters visible from Earth are open star clusters. For example, the Pleiades and the Hyades clusters are open star clusters. Open star clusters are born, and live out their lives, within the galactic disk. They are loose collections of several hundred stars. The ones we know best are relatively nearby, a few hundred light-years away.
In contrast, M5 is a globular star cluster. Globular clusters reside within the galactic halo – a sphere-shape region of the Milky Way that extends above and below the galactic disk. If we liken the disk to a hamburger, then the bun would be the galactic halo. Globular star clusters contain hundreds of thousands of stars, tightly packed in a symmetrical ball. These clusters are our galaxy’s oldest inhabitants. In other words, they formed first, as the galaxy was forming. Spanning 165 light-years in diameter, M5 is one of the larger globular clusters known. It contains more than 100,000 stars, as many as 500,000 according to some estimates.
The relatively young stars of open clusters disperse after hundreds of millions of years. The stars in globular clusters still remain intact after many billions of years.
As you gaze at M5, you’re looking at an object that’s around 13 billion years old, more than twice the age of our solar system, and almost as ancient as the universe itself. Considering that M5 lies some 25,000 light-years distant, we can only imagine what this stellar city would look like if it were at the Pleiades’ distance of 430 light-years!
How to find M5. M5 is located in the constellation Serpens Caput (the Serpent’s Head). It is highest up in the south at about 10 p.m (11 p.m. Daylight Saving Time) in mid-June. Because the stars (and star clusters) return to the same place in the sky some 2 hours earlier with each passing month, it’s highest in the sky around 8 p.m. (9 p.m. Daylight Time) in mid-July.
Using a fist at an arm’s length for a guide, M5 resides a good 2 fist-widths to the southeast of yellow-orange Arcturus, summertime’s brightest star. M5 is also three fist-widths to the east of blue-white Spica, the brightest star in the constellation Virgo.
Plus, M5 is about one fist-width to the north (above) Zubeneschamali. These stars give you at least a rough idea of M5 whereabouts in the heavens.
Practiced skygazers star-hop to M5 by way of two faint yet visible Virgo stars: 109 Virginis and 110 Virginis. They draw an imaginary line from 109 Virginis through 110 Virginis, and go twice the distance to land on the star 5 Serpentis. M5 is only 1/3 degree to the northwest (upper right) of this star. The distance from 109 Virginis to M5 spans about 8 degrees of sky. For reference, the width of 4 fingers at an arm length away approximates 8 degrees.