noun नाम
/ˈæb.səˌlut/
(astronomy) the magnitude that a star would have if it were viewed from a distance of 10 parsecs (32.62 light years) from the earth
(खगोलशास्त्र) धर्तरेसावन १० पार्सेक (३२.६२ उजवाड वर्सां) अंतराचेर नखेत्राक पळयल्यार ताचें व्याप्तीचें प्रमाण आसतलें
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