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Sabik

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35Eta Oph · Ophiuchus

Its story

Sabik’s recognisable prominence stems largely from its position as one of the brightest stars in the Oph constellation. Specifically, it’s known for its steady, unwavering light – a vital presence throughout the night. This star’s apparent brightness, a measure of its luminosity relative to background stars, reveals a magnitude of 2.43, making it a significant feature. These characteristics, combined with its spatial position, allow for clear observation and study for astronomers and stargazers.

Observers typically identify Sabik as a ‘35Eta Oph’ star, recognizing its unique spectral characteristics and observed movements within the larger system of the Milky Way galaxy. It’s a star that commands our attention, exhibiting a consistent light output across considerable temporal ranges.

The star's significance can be seen in the context of historical observation techniques. Due to its steady luminance, the star was considered essential in astronomical cataloging, and remains vital in understanding patterns within stellar distributions.

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Compose this star
FactsHIP 84012
Right ascension
17h 10m 23s
Declination
−15° 43′ 30″
Magnitude
2.43
Data: gaia-dr3