Sky & Telescope - November 2023 - 4
SPECTRUM by Peter Tyson
Outer Limits
IMAGINE LOOKING AT a free-floating ball of gas. What would you
see? Even if the gas had some color or texture to it, you might be
hard-pressed to tell where the surface of the ball begins and ends,
where exterior gives way to interior.
That's exactly our experience when observing the Sun (safely, of
course). Stars throw the whole concept of surface out of whack. A soap bubble
has more of a defined shell than our star does. Indeed, when we observe the
Sun, we're not so much looking at it as into it, albeit not very far.
Fortunately, while the Sun doesn't have a solid surface, it does have a visible
one, the photosphere. Serving as the base of the solar atmosphere, the photosphere
gives itself away - and aids us in delimiting the " surface " - by hosting
a range of distinctive phenomena. (See the stunning images on the cover and in
the corresponding feature on page 14.)
Among these phenomena are sunspots, those dark regions that resemble misshapen
sunflowers. A sunspot's black center, its umbra, and the wispy penumbra
that envelops it lend a sense of a horizontal layer to
what is otherwise ever-roiling plasma. Sunspot umbrae
are darker than their surroundings because they're
comparatively cooler: around 3700°C (6700°F) rather
than the predominant 5500°C (9900°F).
Outside of sunspots, most of the photosphere
A solar flare erupts
from the photosphere
in this image taken by
NASA's Solar Dynamics
Observatory.
consists of granules, which the Daniel K. Inouye Solar
Telescope, the subject of our cover story, captures better
than any telescope before it (see the dramatic image on
page 15). Looking like plasma popcorn, granules sheath
the Sun's entire visible surface, the " popped kernels "
each thousands of kilometers across.
The edge, or limb, of the Sun provides an alternate
sense of a covering, an impression enhanced by limb
darkening: When we look near the rim, we aren't peering
as deeply into the Sun as when we look at the middle. As such, we see only
the slightly cooler outer layers of plasma, which in turn appear slightly darker.
Other, loftier solar features also enhance our inkling of a surface from
which they arose. These include prominences, those dazzling flares of plasma
that extend from the photosphere right up to the corona.
Altogether, the solar spectacles transpiring in and above the photosphere
help us visually grasp the giant ball of gas that is our Sun. Without them, we'd
have a much harder time wrapping our heads around what
essentially doesn't have a wrapping.
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Sky & Telescope - November 2023
Table of Contents for the Digital Edition of Sky & Telescope - November 2023
Contents
Sky & Telescope - November 2023 - Cover1
Sky & Telescope - November 2023 - Cover2
Sky & Telescope - November 2023 - 1
Sky & Telescope - November 2023 - Contents
Sky & Telescope - November 2023 - 3
Sky & Telescope - November 2023 - 4
Sky & Telescope - November 2023 - 5
Sky & Telescope - November 2023 - 6
Sky & Telescope - November 2023 - 7
Sky & Telescope - November 2023 - 8
Sky & Telescope - November 2023 - 9
Sky & Telescope - November 2023 - 10
Sky & Telescope - November 2023 - 11
Sky & Telescope - November 2023 - 12
Sky & Telescope - November 2023 - 13
Sky & Telescope - November 2023 - 14
Sky & Telescope - November 2023 - 15
Sky & Telescope - November 2023 - 16
Sky & Telescope - November 2023 - 17
Sky & Telescope - November 2023 - 18
Sky & Telescope - November 2023 - 19
Sky & Telescope - November 2023 - 20
Sky & Telescope - November 2023 - 21
Sky & Telescope - November 2023 - 22
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Sky & Telescope - November 2023 - 30
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Sky & Telescope - November 2023 - 45
Sky & Telescope - November 2023 - 46
Sky & Telescope - November 2023 - 47
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Sky & Telescope - November 2023 - Cover3
Sky & Telescope - November 2023 - Cover4
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