HERCULES AND HIS MIGHTY GLOBULAR CLUSTERS

Despite being one of the largest star patterns, the constellation itself is relatively dim but can be spotted as they are bordered by brighter constellations

David Prosper

Hercules is one of the standout heroes of Greek mythology, but his namesake constellation can be surprisingly hard to find! Once you find the stars of Hercules, look deeper, barely hidden in the space around his massive limbs and “Keystone” asterism are two beautiful globular star clusters: M13 and M92!

Since the constellation itself is relatively dim but bordered by brighter constellations, you can find the stars of Hercules by looking between the bright stars Vega and Arcturus. They are fairly easy to identify. Vega is the brightest star in the constellation Lyra and one of the three stars that make up the Summer Triangle. Arcturus is the brightest star in the constellation Bootes. You may be able to find Hercules “Keystone” asterism first; this distinct pattern of four stars is traditionally shown as the torso of the great hero.

Fluffy and dense

Globular star clusters appear fluffy, round and dense with stars, similar to a dandelion gone to seed, in contrast to the more scattered and decentralised patterns of open clusters. Open clusters are generally made up of young stars that are gradually spreading apart and found inside our Milky Way galaxy, while globular clusters are ancient clusters of stars that are compact, billions of years old, bound to each other and orbit around our galaxy. Due to their considerable distance, globular clusters are usually only visible in telescopes, but one notable exception is M13, also known as the Great Cluster or Hercules Cluster.

During very clear dark nights, skilled observers may be able to spot M13 without optical aid along the border of the Keystone, in between the stars Zeta and Eta Herculis. Readily visible as a fuzzy “star” in binoculars, in telescopes M13 explodes with stars and can fill up an eyepiece view with its sparkling stars, measuring a little over half the diameter of a full Moon in appearance!

When viewed through small telescopes, globular clusters can appear orb-like and without discernable member stars, similar in appearance to the fuzzy comae of distant comets. That’s why comet hunters Edmund Halley and Charles Messier discovered and then catalogued M13, in 1714 and 1764 respectively. marking this faint fuzzy as a “not-comet” so as to avoid future confusion.

While enjoying your view of M13, don’t forget to also look for M92! This is another bright and bold globular cluster, and if M13 wasn’t so spectacular, M92 would be known as the top celestial sight in Hercules. M92 also lies on the edge of naked-eye visibility, but again, binoculars and especially a telescope are needed to really make it pop.

Far, far away

Even though M92 and M13 appear fairly close together in the sky, in actuality they are rather far apart: M13’s distance is estimated at about 25,000 light years from Earth, and M92’s at approximately 27,000 light years distant. Since M13 and M92 appear so close together in our skies, switching between these two clusters in your scope makes for excellent star-hopping practice.

Globular clusters are closely studied by astronomers for hints about the formation of stars and galaxies. The clusters of Hercules have even been studied by NASA’s space telescopes to reveal the secrets of their dense cores of hundreds of thousands of stars.

(This article is distributed by NASA’s Night Sky Network. Visit nightsky.jpl.nasa.gov for more space news)

ASTRONOMY TERMS

Constellation: a group of stars forming a recognizable pattern

Asterism: a prominent pattern or group of stars that is smaller than a constellation

Keystone: an asterism formed by four relatively bright stars in the constellation Hercules: Pi, Eta, Zeta and Epsilon Herculis

Light year: the distance light travels in one year. Light zips through interstellar space at 3,00,000 km per second and 9.46 trillion km per year

Picture Credit: Google 

Leave a Reply

Your email address will not be published. Required fields are marked *