During the next hour or so, the Moon hides more and more of the Sun and daylight fades, though imperceptibly at first. It’s a leisurely affair, so you have plenty of time to look around. As the eclipse progresses, can you detect any change in the color and quality of the sky, the clouds, nearby objects, and distant landscapes?

Once more than three-quarters of the Sun is covered, the light begins to fade noticeably. By about 15 minutes prior to totality, the light becomes noticeably dimmer and starts to take on an odd or eerie “tint.” Shadows become sharper and more detailed. Look away from the shrinking solar crescent — has there been a change in the color of the sky and clouds since the eclipse began?

As the Sun dwindles to a thin crescent, shadows become much sharper. Look at your own shadow — notice how you can see the shadows of individual hairs on your head or arms.

As the sunlight dims, you may spot the local fauna acting in a peculiar manner. Many start to settle in as if night is falling. Notice the people around you — they’re likely more animated than any local wildlife!

As totality nears, you may notice a perceptible drop in the temperature, and the wind may pick up, die down, or change direction.

Look west a few minutes before totality. Can you see the oncoming umbral shadow? Clouds on the horizon will go dark as the Moon’s shadow sweeps over them, making the approaching umbra more noticeable.

Very dim, undulating ripples of dark and light might appear, flowing across the ground or the side of a white building. These hard-to-see features are caused by atmospheric turbulence and refraction of the thin solar crescent just prior to second contact and/or immediately after third contact.

Some 30 seconds before totality, cover the shrinking solar crescent with your outstretched thumb and remove your eclipse viewers. You’ll likely spot the Sun’s corona (its outer atmosphere) on the side opposite the crescent. But if you do this, you might miss the next two events!

Just prior to totality, all that remains of the Sun are a few shafts of light shining through deep valleys on the lunar limb (edge). The result is a few brilliant beads that disappear one after another. If you’re using a telescope or binoculars to observe the beads, keep your solar filters on until the last bead disappears. If you’re observing only by eye, remove your “eclipse glasses” or solar viewer once the number of beads dwindles to one.

The lunar shadow envelops you. Only a single bead remains — it shines like a brilliant diamond set into a pale ring created by the pearly white corona surrounding the Moon’s black silhouette.

The last bead vanishes; if you haven’t already done so, remove all solar filters now. The brilliant solar surface is hidden, and the Sun’s ghostly, gossamer corona glows around the black lunar silhouette. Feel free to scream and yell in delight, or just stare in silent awe.

For a brief time after the start of totality, the Sun’s chromosphere (thin middle atmosphere) remains visible along the solar limb (edge) still being covered by the advancing Moon. This vivid arc of red vanishes quickly, so don’t miss it. Depending on how active the Sun is, you may spot several streamers of red stretching up from the chromosphere into the corona. These are solar prominences, and they, too, soon disappear behind the encroaching lunar limb.

Now’s the time to explore the solar corona, the star of the show. Using just your eyes, take a few moments to carefully study the appearance of the corona near the Sun. Can you detect any color? Does the corona look smooth or mottled?

Use averted vision (stare at the eclipsed Sun, but concentrate your attention on the corona streaming away from either side of the Sun) to determine how far east and west the faint, outer corona extends. Is it rounded or elongated?

Now use binoculars or a telescope to check out detail within the corona. Look for loops and arcs that reveal solar magnetic fields, and compare the structure of the corona at the Sun’s poles and equator (it’s often quite different).

For the 2028 eclipse, viewing from Sydney, the eclipsed Sun will be at about 30 degrees up from the horizon in the north-west. Brilliant Venus will be low down further to the west and very close to the horizon.

Jupiter (not as bright as Venus) will be higher in the sky and to the right of the Sun. Mercury and Mars will be between the eclipse and Venus but fainter and may be hard to spot.

Looking closely you may see stars including Sirius, Rigel and Regulus. But don’t spend too much time looking for them, totality is fleeting.

To the west along the path of totality the Sun will be more towards north and higher in the sky (up to about 50 degrees above the horizon). Venus will easier to spot being higher in the sky. The other planets and stars will also be higher in the sky and a little more towards the east.

Sky darkness during totality varies from eclipse to eclipse. How dark it gets depends on the Moon’s angular size relative to the Sun’s, the presence or absence of clouds, and how close your site is to the centerline. Just outside the path of totality, the Sun is still shining, albeit dimly. This feeble light creates a beautiful 360° sunrise/sunset glow around the horizon. Don’t miss it.

Beware of spending totality with your eye glued to your camera’s viewfinder. Taking pictures is fine, but make sure you take time to appreciate what is truly a total sensory spectacle. If you’re using a telescope to examine the stunning detail in the corona, pause for a few moments, look away, and absorb the surrounding vista.

Yes, both the sky and the edge of the corona opposite where the Sun vanished really are a little brighter now. Fingers of red (prominences) slowly rise from behind the Moon’s retreating limb. They are soon joined by an emerging arc of red light — the chromosphere. The end of totality is imminent. If you’re looking through optics, now is the time to replace your solar filters!

One blazingly bright bead of sunlight erupts into view. Totality is over. Solar filters on! The stages of the eclipse now repeat in reverse order.

More rays of sunlight burst through lunar valleys and quickly combine to form a very thin crescent. The solar crescent rapidly expands, and the sky brightens quickly. If you want a few more seconds of corona viewing, block the emerging Sun with your thumb.

These dim ripples of dark and light may appear briefly while the extremely thin solar crescent twinkles like a star.

Retreating Shadow If you’re not busy watching for shadow bands or squeezing in a few more seconds of corona viewing, quickly look away from the emerging Sun. Can you see totality’s wave of darkness speeding rapidly into the east?

The temperature will likely continue to cool slightly after totality concludes and begin to rise shortly thereafter. However, the change may be subtle and could be masked by a shift in wind speed and direction.

As the Sun emerges, so too will any birds and animals that, as totality approached, decided something odd was happening and started to get ready for bed. Meanwhile, your eclipse-watching companions will be happily chatting among themselves, comparing images, and probably ignoring the returning solar disk.

While the Sun remains a thin crescent, shadows are much sharper than usual. If you forgot to look at your own shadow on the ground before totality, be sure to look now — you’ll see crisp shadows of hairs on your head or arms.

Just as it took a while for the Moon to cover the Sun, it will take an equally long interval — more than an hour — for the Moon to move off the solar disk. (The time between third and fourth contact will seem much, much longer than between first and second contact!) But don’t lose track of time — you’ll want to witness the official end of the eclipse.

The last tiny indentation on the Sun disappears, and the Moon no longer covers any part of the solar surface. The eclipse is officially over.

Eclipse veterans like to use the phrase “experience totality” rather than “see totality,” because a total solar eclipse is the only celestial phenomenon that truly overwhelms the senses. Most astronomical observing involves straining to perceive something at the limit of visibility — a faint galaxy, a dim double-star companion, or a tiny festoon in Jupiter’s clouds. A solar eclipse is the most extreme exception to this rule. You don’t have to use averted vision, special filters, or other tricks to experience totality. You just have to put yourself in the right place at the right time and hope for clear skies. When the Moon’s shadow arrives, it hits you over the head.

But what if you don’t have clear skies? Unwelcome clouds are always a possibility.

Without doubt, the highlight of any solar eclipse is the gossamer corona, which is visible only if the sky is relatively clear and transparent. But many of the other phenomena described above can be experienced even if clouds cover the Sun. For example, it will get dark, the temperature will go down, any wildlife or domesticated animals in the area will exhibit changes in behavior, and your fellow eclipse watchers will make sounds — though perhaps not happy ones.

You can take some comfort from remembering that even under perfectly clear skies, it’s impossible for a single observer to take in everything that happens during a total solar eclipse. You can’t look up in the sky at the last sliver of Sun at the same time you’re looking down at the ground for shadow bands. You can’t admire the pretty sunrise/sunset colors around the horizon while you’re examining coronal streamers in a telescope. So even in ideal conditions, you end up seeing some things that others miss, and missing some things that others see. That’s why some people seek to experience totality again and again.