- distinguish between a solar eclipse and a lunar eclipse
- describe why safety precautions must be taken when observing a solar eclipse or transit
Partial Solar Eclipse
something, is to cause a partial or total obscuring of an object. In
astronomical terms, our “objects” are the Sun, Moon and Earth. This
gives us two kinds of eclipses visible from the Earth: solar eclipses
, where the Sun is blocked, and lunar eclipses
where the Moon is blocked.
solar eclipse occurs when the Moon comes exactly between the Sun's rays
and the Earth, blocking the Sun and creating a period of darkness on
the Earth. The Moon actually comes close to blocking the Sun once every
28 days, during a New Moon (see Module 4, Tutorial 3), but not quite.
This is due to the Moon’s orbit being tilted about 5? to the ecliptic,
meaning the Moon often passes just north or just south of the Sun,
without blocking it. When the Sun and the Moon line up perfectly,
though, a total eclipse
where the Sun is completely blocked from our view. Total solar eclipses
happen roughly once or twice a year, and offer spectacular sights: with
the disk of the Sun completely blocked, astronomers can see the halo of
gas surrounding the Sun called the corona.
Total solar eclipse as seen from Turkey, March 29, 2006. The
perfectly blocks the disk of the Sun, allowing the corona to be viewed.
Credit & Copyright: Koen van Gorp
Essentially what occurs is that the Moon is casting a shadow on a part
of the Earth. Since the moon is small compared to the Earth the shadow
only covers a small part of the Earth. This makes total solar eclipses
visible only from specific locations on the Earth, depending how the
Moon lines up with the Sun. These locations vary from eclipse to
eclipse; Canada will see its next total solar eclipse in the year 2024.
From other locations on Earth, the Moon only covers part of the Sun,
and a partial eclipse occurs. During a partial eclipse
, part of the Sun’s disk remains visible at all times.
The shadow of the moon on the Earth during an eclipse. The latitude
and longitude lines are added for reference. A total solar eclipse would
only be visible if you are standing within the darkest part of the shadow.
A third type of solar eclipse, called an annular eclipse, occurs when
the Moon is at apogee – the point in its orbit where it is the furthest
from the Sun (see Module 4, Tutorial 1). Because it is further from the
Earth, the Moon appears to be smaller, and hence doesn’t cover he
entire disk of the Sun. As a result, at the moment of greatest eclipse
the Moon covers the centre of the Sun, and is surrounded by a ring of
When the Moon lines up exactly with the Sun and only blocks part of it,
Did you know?
result is an annular eclipse. This image was taken during the 2005
eclipse as seen from Spain.
live in a very fortunate time, in terms of viewing solar eclipses. The
diameter of the Sun is approximately 400 times larger than the Moon,
but the Moon is about 400 times closer to the Earth than the Sun, which
means that during a total eclipse, the Moon perfectly blocks the disk
of the Sun. As the Moon moves further away from the Earth (see Module
4, Tutorial 1), generations far in the future will only see the Moon
cover most of the Sun during a total eclipse
was the sight of a total solar eclipse in 1925 which helped convince
renowned Canadian astronomer Dr. Helen Sawyer-Hogg to pursue a career
in astronomy. Dr. Sawyer-Hogg was quoted as later saying, about the
eclipse, “the glory of the spectacle seems to have tied me to astronomy
for life, despite my horribly cold feet as we stood almost knee deep in
the snow.” She became a teaching assistant at the University of Toronto
in 1936, and began teaching there in 1941, eventually becoming a full
professor in 1956. Dr. Sawyer-Hogg was known for her research on
variable stars in globular clusters. She discovered hundreds of
variables and published more than 200 papers, publishing three editions
of Catalogues of Variable Stars in Globular Clusters
in 1939, 1955, and 1973. To most Canadians, she was probably best known
for her work in public education. For thirty years, she wrote a weekly
column entitled With the Stars
for the Toronto Star.
She was also the founding President of the Canadian Astronomical
Society when it formed in 1971. All this from the sight of an eclipse!
During a lunar eclipse, it is the Earth that gets in
the way. Typically, we can see the Moon at night because of the
sunlight which is reflected off of it. Depending on where the Moon is
relative to the Sun, we see difference phases (see Module 4, Tutorial
3). However, when the Moon is in just the right place, the Earth passes
directly between the Sun and the Moon, preventing all of the Sun’s
light from reaching the Moon.
Moon, however, never becomes completely invisible, due to some of the
Sun’s light being refracted by the Earth’s atmosphere (see Module 3,
Tutorial 2). This refracted light gives the Moon a dim, red appearance.
During a lunar eclipse, refracted sunlight makes the dim Moon
appear red in colour.
Often, solar and lunar eclipses occur in equal numbers in any given
year. The maximum number of eclipses (solar and lunar combined), which
can occur in one year is seven, as was observed in 1982. The next year
for a combination of seven eclipses will be 2038.
Rarely, a third kind of eclipse can be seen from the Earth – a transit:
when a planet closer to the Sun (in our case, Venus or Mercury) passes
in front of the Sun, blocking part of the Sun’s light. Because the
planets are much farther from the Earth than the Moon, they only block
a tiny part of the Sun, appearing as a black dot moving across the
When the Moon passes in front of the Sun, most of the Sun gets blocked.
When Mercury passes in front of the Sun, its small size blocks only a tiny
part of the Sun! Mercury is visible as a small black dot toward the centre
of the Sun.
Transits of Venus happen very rarely. The next one
will occur in 2012, but then not again until 2117. Transits of Mercury
are more common, occurring 13 or 14 times per century. Future transits
of Mercury will occur in 2016, 2019, 2032 and 2039. Transits of Mercury
occur more frequently because Mercury orbits the Sun much more quickly
than Venus, giving us more opportunities to view transits.
people remember solar eclipses as times when parents told children to
stay inside, recess was cancelled at school and the curtains drawn, so
that children wouldn’t stare at the eclipse and risk damaging their
eyes. But is staring at an eclipse any more dangerous than staring at
The answer is both yes
and no. It is a well-known fact that looking into the Sun with the
naked eye (and especially with binoculars or a telescope) can cause
irreversible damage to the nerves in your eye. We have a natural
defense mechanism to protect our eyes – we squint! During a solar
eclipse, as the Moon is moving in front of the Sun, the Sun’s rays are
just as harmful as they normally are, but this time, as the Moon blocks
more and more of the light, we don’t feel the need to squint as much,
and more of the Sun’s damaging radiation can make it into our eyes.
Check It Out!
There are a number of ways to safely view a solar eclipse or transit. Look up the projection method, solar viewing glasses
and safe solar filters online
using your favourite search engine to learn more about the different techniques