New NASA research reveals a process to
generate extremely accurate eclipse maps, which plot the predicted path of the
Moon’s shadow as it crosses the face of Earth. Traditionally, eclipse
calculations assume that all observers are at sea level on Earth and that the
Moon is a smooth sphere that is perfectly symmetrical around its center of
mass. As such, these calculations do not take into account different elevations
on Earth or the Moon’s cratered, uneven surface.
For slightly more accurate maps, people can employ elevation tables and
plots of the lunar limb — the edge of the visible surface of the Moon as seen
from Earth. However, now eclipse calculations have gained even greater accuracy
by incorporating lunar topography data from NASA’s LRO (Lunar Reconnaissance Orbiter) observations.
Using LRO elevation maps, NASA visualizer Ernie Wright at NASA’s Goddard
Space Flight Center in Greenbelt, Maryland, created a continuously varying
lunar limb profile as the Moon’s shadow passes over the Earth. The mountains
and valleys along the edge of the Moon’s disk affect the timing and duration of
totality by several seconds. Wright also used several NASA data sets to provide
an elevation map of Earth so that eclipse observer locations were depicted at
their true altitude.
The resulting visualizations show something never seen before: the true,
time-varying shape of the Moon’s shadow, with the effects of both an accurate
lunar limb and the Earth’s terrain.
“Beginning with the 2017 total solar eclipse, we’ve been publishing maps and movies of eclipses that show the true shape of the Moon’s central shadow — the umbra,” said Wright.
A map showing the umbra (the Moon’s central shadow) as
it passes over Cleveland at 3:15 p.m. local time during the April 8, 2024,
total solar eclipse.
NASA SVS/Ernie Wright and Michaela Garrison
“And people ask, why does it look
like a potato instead of a smooth oval? The short answer is that the Moon isn’t
a perfectly smooth sphere.”
The mountains and valleys around
the edge of the Moon change the shape of the shadow. The valleys are also
responsible for Baily’s beads and the diamond ring, the last bits of the Sun
visible just before and the first just after totality.
A computer simulation of Baily’s beads during a total
solar eclipse. Data from Lunar Reconnaissance Orbiter makes it possible to map
the lunar valleys that create the bead effect.
NASA SVS/Ernie Wright
Wright is lead author of a paper published Sept. 19 in The Astronomical Journal
that reveals for the first time exactly how the Moon’s terrain
creates the umbra shape. The valleys on the edge of the Moon act like pinholes projecting images of the Sun onto the Earth’s
surface.
A visualization of Sun images being projected from
lunar valleys that are acting like pinhole projectors. Light rays from the Sun
converge on each valley, then spread out again on their way to the Earth.
NASA SVS/Ernie Wright
The umbra is the small hole in the
middle of these projected Sun images, the place where none of the Sun images
reach.
Viewed from behind the Moon, the Sun images projected
by lunar valleys on the Moon’s edge fall on the Earth’s surface in a
flower-like pattern with a hole in the middle, forming the umbra shape.
NASA SVS/Ernie Wright
The edges of the umbra are made up
of small arcs from the edges of the projected Sun images.
This is just one of several
surprising results that have emerged from the new eclipse mapping method
described in the paper. Unlike the traditional method invented 200 years ago,
the new way renders eclipse maps one pixel at a time, the same
way 3D animation software creates images. It’s also similar to the way other
complex phenomena, like weather, are modeled in the computer by breaking the
problem into millions of tiny pieces, something computers are really good at,
and something that was inconceivable 200 years ago.
For more about eclipses, refer to:
https://science.nasa.gov/eclipses
By Ernie Wright and Susannah
Darling
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Source: NASA Develops Process to Create Very Accurate Eclipse Maps - NASA Science
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