Out-of-Bounds Venus
Taste drifts away from its usual standards, making unfamiliar people and styles more attractive. Test one choice on a small scale before making a lasting commitment.
In detail
Venus out of bounds occurs when transiting Venus moves beyond the Sun's declination limit of about 23°26′ north or south, starting at the outward crossing and ending at re-entry. Venus travels about 1° per day, giving a 3° monitoring band around either boundary crossing a span of roughly five to six days; retrograde motion may produce repeated passages, but the complete interval is fixed by the actual crossings. Venus governs attraction, exchange in relationships, and aesthetic preference, so outside the solar range its choices become less accountable to familiar or collective standards. A declination parallel requires two bodies to align on the same side, while Venus out of bounds depends only on Venus exceeding the solar limit.
FAQ
- How long does out-of-bounds Venus last?
- There is no fixed duration. It starts when Venus crosses beyond the Sun's declination limit and ends when Venus returns inside it, so the exact dates must be checked in the current ephemeris rather than inferred from a single day.
- Is out-of-bounds Venus the same as a Venus parallel?
- No. Out-of-bounds Venus concerns Venus crossing the Sun's declination limit on its own, while a parallel requires Venus and another body to share the same declination; one describes an unusual Venus mode, and the other links two planetary themes.