Global reference time: December 21, 2028 at 08:19 UTC. Your local calendar date may differ.
This marks a seasonal boundary, rather than a brief visible sky event.
What to expect
Visibility & observing notes
A seasonal milestone that occurs at one global instant, with opposite seasons in the two hemispheres.
Northern Hemisphere
Winter
Southern Hemisphere
Summer
Understand the moment
A tilted Earth makes the seasons
The geometry behind December Solstice
Earth’s rotation axis is tilted about 23.4 degrees from the perpendicular to its orbital plane. As Earth travels around the Sun, that tilt changes sunlight angle and day length in each hemisphere, producing opposite seasons in the north and south.
Opens . Each scene is an exact daily sample, without interpolation; it is separate from the catalog peak of 08:19 UTC.
How to read the scene: This orbital lesson does not calculate local day length or use the globe’s illustrative surface orientation to reproduce an equinox or solstice. The event time above is the exact catalog milestone.
More about observing seasons
A little context. A better view.
Equinoxes & Solstices: a field guide
01
Astronomical seasons have precise boundaries
Equinoxes and solstices are calculated from the Earth–Sun geometry. Their exact times are global; the local calendar date can differ by time zone.
02
The hemispheres tell opposite stories
A June solstice marks the start of astronomical summer in the Northern Hemisphere and winter in the Southern Hemisphere. Event details identify both hemispheres.
03
These are calendar milestones
An equinox or solstice is not a brief object appearing in the sky. No special equipment or clear weather is required to mark the instant in your calendar.
04
Weather seasons are a different convention
Astronomical season boundaries do not predict a particular temperature or a sudden weather change. Local climate and seasonal weather follow their own patterns.