The Constellation Serpens Caput

by Dominic Ford
Serpens Caput Serpens Caput
The constellation Serpens Caput. Roll mouse over to see labels.
Source: Stellarium.

Serpens is unique among the constellations in that it is divided into two separate pieces which are considered part of the same constellation.

It represents a snake which is usually depicted either wrapped around the waist of Ophiuchus the serpent bearer, or else wrapped behind his back.

When Eugène Delporte came to define the modern constellation boundaries in the 1920s, he faced the problem of how to separate the serpent and serpent-bearer into two separate constellations, and he opted to split the serpent into two parts.

Serpens is an equatorial constellation which appears highest in the evening sky in the months around June.

Both the head of the snake, Serpens Caput, and the tail of the snake, Serpens Cauda are represented by third and fourth magnitude stars

The head of the snake is well separated from the Milky Way, and contains no bright deep sky objects. The tail of the snake, however, not only lies close to the plane of the Milky Way, but also neighbors Sagittarius, the constellation which contains the galaxy's center. It is home to several bright open clusters and globular clusters.

Serpens is not the only snake in the night sky, and neither is it the largest. The largest of all the constellations is Hydra, the water snake, which also has a smaller and fainter companion in the far-southern sky, Hydrus.

Date First Appeared
Ancient
Sky Area
1.5% of the sky
636.9 square degrees
Messier Objects
Serpens Caput contains the following Messier object: M5.
Caldwell Objects
Serpens Caput contains no Caldwell objects
Neighbors
The following constellations neighbor Serpens Caput: Bootes, Corona Borealis, Hercules, Libra, Ophiuchus, Virgo.
Please wait
Loading 0/4
Click and drag to rotate
Mouse wheel to zoom in/out
Touch with mouse to dismiss

Brightest Objects in Serpens Caput

Stars Open Clusters Globular Clusters Galaxies
Stars Open Clusters Globular Clusters Galaxies
Unukalhai (mag 2.6) Messier 5 (mag 5.8) NGC 5921 (mag 10.8)
μ-Ser (mag 3.5) NGC 5970 (mag 11.4)
β-Ser (mag 3.6) NGC 5962 (mag 11.4)
ε-Ser (mag 3.7) NGC 6070 (mag 11.7)
δ-Ser (mag 3.8) NGC 6118 (mag 12.0)
γ-Ser (mag 3.9) NGC 5936 (mag 12.4)
κ-Ser (mag 4.1) NGC 6027 (mag 12.4)
δ-Ser (mag 4.1) NGC 6020 (mag 12.6)
λ-Ser (mag 4.4) NGC 6010 (mag 13.0)
ι-Ser (mag 4.5) NGC 5951 (mag 13.0)
ρ-Ser (mag 4.7) NGC 5957 (mag 13.0)
π-Ser (mag 4.8) NGC 5964 (mag 13.0)
σ-Ser (mag 4.8) NGC 5990 (mag 13.0)
MQ Ser (mag 5.1) NGC 5996 (mag 13.0)
b-Ser (mag 5.1) NGC 6004 (mag 13.0)
HD 71115 (mag 5.1) NGC 5937 (mag 13.0)
10-Ser (mag 5.2) NGC 6012 (mag 13.0)
τ¹-Ser (mag 5.2) NGC 5984 (mag 13.0)
ω-Ser (mag 5.2) NGC 5953 (mag 13.0)
16-Ser (mag 5.3) NGC 5956 (mag 13.0)
χ-Ser (mag 5.3) IC 1151 (mag 13.0)
3-Ser (mag 5.3) IC 1158 (mag 13.0)
A²-Ser (mag 5.4) NGC 6051 (mag 13.0)
HD 145206 (mag 5.4) NGC 5980 (mag 13.0)
6-Ser (mag 5.4) NGC 5920 (mag 13.6)

Ashburn

Latitude:
Longitude:
Timezone:

39.04°N
77.49°W
EDT

Color scheme