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Rasalas

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24Mu Leo · Leo Minor

Its story

Rasalas is easily identifiable through its placement within the constellation LMi. Its observed brightness, averaging 3.53, strongly points to a Cepheid variable star – a pivotal type of star with a predictable luminosity tied to its pulsation period. The consistent timing of its pulsating brightness allows astronomers to measure distances with exceptional precision using standard astronomical measurements. Observations conducted over a period of 7.2 days, the star’s intrinsic luminosity is approximately 2.88 Solar Luminosity or 1.4 x 10^4 L<sub>solar</sub>. The calculated luminosity has an average value of 2.89 L<sub>solar</sub>.

For many astronomical observers, Rasalas, is chosen as a symbolic dedication. A gentle beacon in the heavens, mirroring a steady, unchanging rhythm – hinting at a foundational harmony, perhaps representing longevity and steadfastness. Its prominence within the LMi constellation warrants thoughtful consideration among stellar systems.

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Compose this star
FactsHIP 48455
Right ascension
9h 52m 46s
Declination
+26° 00′ 24″
Magnitude
3.53
Distance
≈ 125 ly
Data: gaia-dr3