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A Closer Look: Angular Size

Kathy Price's class uses angular
size to measure the relative size of the Moon. |
Unlike most sciences, astronomers are generally unable to travel or to
directly interact with the objects that they study, so it can
be difficult to determine the distance to those sources. Among other tools,
astronomers
use geometry to estimate these distances.
Objects in the sky can
be described by their angular size, which is how big they look,
or their physical size, which is how big
they are. How big an object looks depends on both how big it
is and how far away
it is. For instance, when looking at the Moon in the sky, it
has an angular diameter of half a degree. This angular size is
determined by the physical
size of the Moon, and the distance to the Moon. If the Moon were
twice as far away, it would look half as big, and if the Moon
were twice a large,
it would look twice as big. Once astronomers know an objects
physical size — which they can determine through a variety of techniques — they
can easily measure its angular size. Those two measurements allow
them to determine how far away an object is. For instance, in
this video, the
students learn that the Moon appears half as wide as their pinky
when held at arm's length. They also learned that when standing
on the Moon,
Earth appears as wide as two fingers held at arm's length. Using
this knowledge, plus knowing the diameter of the Earth, they
can calculate the physical size of the Moon and the distance between Earth
and the Moon.
Astronomers can use parallax to determine the distance to
objects
in the sky. As Earth orbits the Sun, we observe nearby stars
from slightly different angles. By measuring how much the position
of a star appears
to shift (the parallax angle), astronomers can determine the
distance to that star. To understand this, close one eye and
hold a finger in front
of your face. Now, alternate which eye is open and which eye
is closed, and you will see that it appears as if your finger
is changing position.
As you move your finger closer to your face, the amount of
change becomes larger. Just as you can estimate the distance to your hand
by
the amount
by which your finger appears to move, astronomers can estimate
the distance to objects in the sky by measuring the apparent
change in position of
the objects they study during different parts of Earth's orbit.
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