Daylight Hours in Antarctica: Autumn & Spring Transition Explained
Antarctica's extreme latitude creates the planet's most dramatic seasonal light cycles. At the South Pole (90°S), there is only one "day" and one "night" per year—each six months long. Coastal stations experience less extreme but still profound transitions.
Autumn (March – May): The Long Fade
- March 21 (Autumn Equinox): Sun circles horizon, 12 hrs day/night everywhere.
- Late March – April: Sun dips below horizon at pole; coastal stations lose ~20–30 min/day.
- May: Civil twilight (sun <6° below horizon) persists at coast; pole enters full darkness.
- June 21 (Winter Solstice): Maximum darkness. Pole: 24-hr night. Coast (e.g., McMurdo 78°S): ~4–6 hrs civil twilight; no true sunrise.
Spring (September – November): The Long Return
- September 23 (Spring Equinox): Sun returns to horizon at pole; 12 hrs day/night globally.
- Late Sept – Oct: Coastal stations gain ~20–30 min/day; pole in continuous twilight.
- November: Sun rises at pole (Sept 21–23); climbs higher daily. Coast: 18–24 hrs daylight by late Nov.
- December 21 (Summer Solstice): 24-hr daylight at pole; coast: midnight sun.
Coastal Examples (2024)
| Station | Lat | Mar 21 | Jun 21 | Sep 23 | Dec 21 |
| McMurdo (US) | 78°S | 12h | Twilight only | 12h | 24h |
| Rothera (UK) | 67°S | 12h | ~2h daylight | 12h | 24h |
| Palmer (US) | 64°S | 12h | ~4h daylight | 12h | 20h+ |
Key takeaway: Autumn = rapidly diminishing light → polar night. Spring = rapidly increasing light → midnight sun. The transitions are swift (weeks), not gradual like mid-latitudes.