Zenith

arabic: سمت الرأس (samt al-raʾs) · greek: κατὰ κορυφήν (kata koryphēn, 'directly overhead') · babylonian: ziqpu (Akkadian) — meridian-overhead reference stars

Definition

Zenith is the astronomical point on the celestial sphere directly overhead at the observer's location — the local 90°-altitude point of the horizontal coordinate system. Its opposite point, directly below the observer, is the nadir. In Babylonian observational astronomy the ziqpu stars cross the zenith at upper culmination as meridian timing-references through the night. In Egyptian archaeoastronomy zenith pass — the moment the Sun crosses exactly overhead at a given latitude — anchors the calendar. In Western astrology the zenith is sometimes loosely used as a synonym for the Midheaven, though strictly the two points are distinct.

In Tradition

Across Egyptian, Babylonian, and Hellenistic-Western traditions the zenith is the foundational overhead-reference of horizon-coordinate astronomy. Hunger & Steele's MUL.APIN documents the ziqpu stars as 'a star at the celestial meridian — the point directly overhead.' Rochberg's *Heavenly Writing* characterises ziqpu stars as 'bright reference stars that cross the zenith of the observer.' Belmonte and Lull define zenith pass as 'the astronomical event whereby a celestial body passes exactly overhead at a particular latitude.'

In Practice

Practitioners use the zenith in two distinct contexts. First, in archaeoastronomy and observational astronomy: Babylonian astronomers identified a canonical fourteen ziqpu stars (per MUL.APIN Tablet I iv 1-9) whose successive transits of the meridian let them time the risings and settings of all other stars through the night; Egyptian astronomers at Aswan / Elephantine c. 3000 BC used the solar zenith-pass (at 24°5′ solar declination, exactly the latitude of central Aswan) to establish the 365-day year length, supplanting Neugebauer's older Nilothic hypothesis. Second, in modern Western astrological practice: the zenith is sometimes spoken of loosely as the Midheaven, though the astronomical zenith (90° from the horizon at the observer's location) and the astrological MC (the ecliptic-meridian intersection) coincide only under restricted geometric conditions. Modern fixed-star paran work uses the zenith and nadir as two of the four cardinal cross-points alongside the rising and setting horizon-points.

Historical Origin

The earliest substantive attestation is Egyptian Old Kingdom calendar work at Aswan / Elephantine c. 3000 BC, where the solar zenith pass at the era's Tropic of Cancer anchors the year-length (Belmonte 2003a, 2009). The Babylonian ziqpu-star meridian-observation system is codified in MUL.APIN Tablet I iv 1-9 and elaborated in Neo-Assyrian, Neo-Babylonian, and Seleucid catalogues. The Greek tradition inherits the overhead-point concept (kata koryphēn); medieval Arabic astronomy gives the word zenith (samt al-raʾs) that English ultimately inherits.

Etymology

Origin: Arabic. Meaning: Direction of the head, overhead point.

Further Reading

  • Juan Antonio Belmonte & José Lull, Astronomy of Ancient Egypt
  • Hermann Hunger & John Steele, MUL.APIN
  • Francesca Rochberg, The Heavenly Writing