Hamal appears as a relatively dim star within the Ari constellation. Measuring at magnitude 2.01, it’s not exceptionally bright, marking a point of moderate distance in the night sky. Hamal has been observed as a fairly consistent object, providing a ste
Known primarily for its visual presence, Hamal has solidified its recognition in the cosmos through its position relative to the Milky Way. Its proximity to the galactic center allows observers, at least in the Northern Hemisphere, to easily spot the star. This connection to the larger galactic flow contributes significantly to its observable prominence.
Historically, Hamal has garnered a significant reputation as a reliable marker for navigation and charting. The star's stability in observing locations across millennia provides a consistent background, allowing historians to study celestial movements. It serves a clear, demonstrable presence in the celestial sphere.
Considering the star's location, Hamal possesses a certain elegance and steadfastness, a compelling visual statement against the vast canvas of the night. It’s a small but notable, enduring brightness – often a gentle beacon amidst the darkness.
How to see it
Hamal has a visual magnitude of about 2.01: under a reasonably dark sky it is typically reachable with the unaided eye.
Sky position
Equatorial coordinates for Hamal: right ascension 2h 7m 10s, declination +23° 27′ 45″ (J2000), on the celestial sphere.
Catalog context
Hamal. It appears in classical and modern catalogs as Bayer/Flamsteed designation 13Alp Ari, HIP 9884, HD 12929, Gaia DR3 HYG-HIP-9884.
Catalog identifiers
- Gaia
- Gaia DR3 HYG-HIP-9884
- HIP
- 9884
- HD
- 12929
- gaia_dr3
- HYG-HIP-9884
- Bayer / Flamsteed
- 13Alp Ari
Also known as
- 13Alp Ari
- Gaia DR3 TOP 5M HYG-HIP-9884
- Gl 84.3
- HD 12929
- HIP 9884
- HYG-HIP-9884
Observed properties
- Visual magnitude
- 2.01