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1. Note the Sun’s position rising—over five times its width every week.

Each day, the Sun moves eastward against the stars. Being in Aquarius, it simultaneously has a northern component that yields this elevation rise. Sky watchers perceive this, and welcome the heightened rays, especially because the loftier angle increases sunlight’s skin-warming infrared component.

Yet for most, the change is too slow to be noticed. You can’t blame anyone. Our culture prizes speed. Many can recite the cheetah’s 70-mile-per-hour capability while far fewer know that sloths, those dawdling archetypes, lope along at 0.07 mph, a thousand times slower. We tend to ignore sluggish things. 

Backyard telescope owners see this when entertaining visitors. They’re impressed if we explain that the hum they hear is the telescope tracking the Moon as it crosses the sky. Interest flags when they realize that following any celestial object merely requires that the motor perform a one-revolution-per-day.

See my article to learn more about the Sun’s climb in spring.

2. Yes, we can see Earth’s spin with the naked eye.

Award yourself an acre on the Moon if you said yes. Because of course, you can perceive Earth’s rotation. 

When watching the setting Sun, you’ve certainly observed it slowly bury itself into the ocean horizon. And the Sun’s red final upper pinpoint, which some of us always hope will briefly turn emerald and gift us with a “green flash,” visibly vanishes all too quickly. 

So happens, the setting Sun and Moon pretty much match the apparent visual speed of a minute hand’s pointy tip on a wall clock. It’s right on the edge of appearing stationary, but if you’re patient you’ll definitely detect its motion. That our planet spins at such a rate is fascinating, even if we’ve grown used to it. 

See my article on how fast the Earth spins and why we don’t feel it.

Mars almost exactly matches our rotation speed, while Jupiter’s equator zooms 25 times faster than ours. On the other hand, our nearest planet neighbor Venus has a spin speed of just ten miles an hour, so you’d never visibly detect a sunset from there, even if it wasn’t always overcast.

3. We can visibly detect the Moon’s orbit.

Such slow speeds can actually manage to be exciting.

The Moon in its orbit lopes along at one kilometer per second, which makes its entire disk fully shift position in space in one hour, making it the only known celestial body that moves exactly one of its widths per hour. 

We’ll see this very phenomenon if we observe April’s solar eclipse since the Moon will require one hour to fully cover the Sun, from start to finish. Or, for that matter, for the Moon to wholly enter Earth’s shadow during any lunar eclipse. So, yes, we’ve already derived excitement from the Moon’s leisurely orbit.

4. Even dust bunnies and flower blossoms are moving

It’s all around us on Earth too. 

• Bedroom dust hanging in the air, illuminated by shafts of sunlight, settles at the rate of an inch an hour. 
• The continental plate we’re on typically moves an inch a year. The fastest, carrying Hawaii northwest, zooms at four inches a year. 
• The quickest bacteria sprint the width of a human hair in a mere second, which lets them cross a damp kitchen counter in an hour. (No wonder diseases spread.) 
• And during the next month or two, springtime’s awakening of blossoms moves poleward at 0.6 mph, or one kilometer per hour, about the rate of a parent pushing a stroller. 

That’s a wonderful image—that tree buds opening into leaves is a process that creeps northward at the rate of a slow walk. 

5. Watch the stars above which reveal Earth’s shifting poles

But if your focus is the absolutely most leisurely celestial phenomena that have managed to grab human attention, you could start with the ancient Greek Hipparchos back in 129 BC, who realized that star positions had slightly changed since the charts of the earlier Babylonians.

This precession of the poles makes spring equinoxes move slowly westward against the fixed stars. The rate is extremely slow in Earth time; the poles slowly shift in a 27,780-year cycle. But precession explains why people sang about the dawning of the age of Aquarius when the spring equinox—when the Sun annually stands momentarily over the equator—nowadays happens against the stars of Taurus the Bull. 

6. But what about you and me? 

Do we ever focus on minuscule motion? Rarely. The only plant that grows fast enough to be seen to visibly change is bamboo. 

Got two hours? Planet Jupiter is the brightest “star” out early these nights. You’ll see its moon Io, and its shadow slide across Jupiter’s cloud-covered disk. In reality, they’re moving at a rate of 25 arcseconds per hour, a motion 2,000 times slower than the setting Sun. 

Of course, it wouldn’t have been detectable without a telescope. Still, it reveals that despite our hurry-up culture, some of us have let astronomy help us “chill out.”

7. Enjoy the increasing daylight—only a minute per day (soon two)

Speaking of chill, the most obvious and life-affecting winter change these days is in the length of daylight. We had our earliest sunset (darkest afternoon) on December 7, and then saw our darkest morning (latest sunrise) during the first week of January.

How it all fits together to deliver hours and minutes of daylight boils down to the very darkest day being the recent solstice on December 21. 

See my article on how daylight changes after the solstice.

The increase in sunlight was just a few seconds per day at first. In late January, the gain in daylight reached more than a minute per day. 

But it’s now changing quickly. In just a few weeks, we’ll be gaining over two minutes of daylight each and every day! 

When it reaches three minutes per day by the end of February, it’ll remain glued to that same rapid sunshine-growth right through April.

And that’s the visible change the greatest number of us will be aware of. We won’t even care when June and July glue that darkness/daylight ratio in place so that, until late in summer, there’s barely any further change to observe.