The Orbit of the Sun, the Measure of Day and Night, and the Sun-God’s Chariot
तत्रत्यानां दिवसमध्यङ्गत एव सदाऽऽदित्यस्तपति सव्येनाचलं दक्षिणेन करोति ॥ ८ ॥ यत्रोदेति तस्य ह समानसूत्रनिपाते निम्लोचति यत्र क्वचन स्यन्देनाभितपति तस्य हैष समानसूत्रनिपाते प्रस्वापयति तत्र गतं न पश्यन्ति ये तं समनुपश्येरन् ॥ ९ ॥
tatratyānāṁ divasa-madhyaṅgata eva sadādityas tapati savyenācalaṁ dakṣiṇena karoti; yatrodeti tasya ha samāna-sūtra-nipāte nimlocati yatra kvacana syandenābhitapati tasya haiṣa samāna-sūtra-nipāte prasvāpayati tatra gataṁ na paśyanti ye taṁ samanupaśyeran.
須弥山に住む者たちは、太陽が常に頭上にあるため、いつも正午のように熱い。太陽は星宿に向かって反時計回りに進み、須弥を左に置くが、ダクシナーヴァルタの風の影響で、時計回りに進み須弥を右に置くかのようにも見える。太陽が昇る地点の直径反対の国では同時に沈むのが見え、正午の地点の反対側では真夜中となる。同様に、日没の地の人が反対の国へ行けば、太陽を同じ状態では見ない。
This verse explains that, for certain regions, the Sun appears perpetually at midday due to relative position—showing Bhagavatam’s cosmological explanation of varying day-phases.
In Canto 5, Śukadeva teaches Parīkṣit Mahārāja the structure and functioning of the universe, including how the Sun’s course relates to time (day, night, noon) for different inhabitants.
It encourages humility and broader vision—what seems ‘fixed’ from one viewpoint can differ elsewhere—supporting patience, perspective, and faith in the Lord’s ordered creation.