Orion starmax 90 eq 사용자 설명서
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Similarly, to point the telescope directly south, the counter‑
weight shaft should again be horizontal. Then you simply
rotate the scope on the Dec. axis until it points in the south
direction.
What if you need to aim the telescope directly north, but
at an object that is nearer to the horizon than Polaris?
You can’t do it with the counterweight down as pictured in
Figure 1. Again, you have to rotate the scope in R.A. so the
counterweight shaft is positioned horizontally. Then rotate
the scope in Dec. so it points to where you want it near the
horizon.
To point the telescope to the east or west, or in other
directions, you rotate the telescope on its R.A. and Dec.
axes. Depending on the altitude of the object you want to
observe, the counterweight shaft will be oriented some‑
where between vertical and horizontal.
Figure 6 illustrates how the telescope will look pointed at
the four cardinal directions ‑ north, south, east, and west
The key things to remember when pointing the telescope is
that a) you only move it in R.A. and Dec., not in azimuth or
latitude (altitude), and b) the counterweight and shaft will
not always appear as it does in Figure 1. In fact, it almost
never will!
weight shaft should again be horizontal. Then you simply
rotate the scope on the Dec. axis until it points in the south
direction.
What if you need to aim the telescope directly north, but
at an object that is nearer to the horizon than Polaris?
You can’t do it with the counterweight down as pictured in
Figure 1. Again, you have to rotate the scope in R.A. so the
counterweight shaft is positioned horizontally. Then rotate
the scope in Dec. so it points to where you want it near the
horizon.
To point the telescope to the east or west, or in other
directions, you rotate the telescope on its R.A. and Dec.
axes. Depending on the altitude of the object you want to
observe, the counterweight shaft will be oriented some‑
where between vertical and horizontal.
Figure 6 illustrates how the telescope will look pointed at
the four cardinal directions ‑ north, south, east, and west
The key things to remember when pointing the telescope is
that a) you only move it in R.A. and Dec., not in azimuth or
latitude (altitude), and b) the counterweight and shaft will
not always appear as it does in Figure 1. In fact, it almost
never will!
6. using Your telescope—
astronomical observing
choosing an observing site
When selecting a location for observing, get as far away as
possible from direct artificial light such as street lights, porch
lights, and automobile headlights. The glare from these lights
will greatly impair your dark‑adapted night vision. Set up on
a grass or dirt surface, not asphalt, because asphalt radiates
more heat. Heat disturbs the surrounding air and degrades
the images seen through the telescope. Avoid viewing over
rooftops and chimneys, as they often have warm air currents
rising from them. Similarly, avoid observing from indoors
through an open (or closed) window, because the tempera‑
ture difference between the indoor and outdoor air will cause
image blurring and distortion.
If at all possible, escape the light‑polluted city sky and head
for darker country skies. You’ll be amazed at how many more
stars and deep‑sky objects are visible in a dark sky!
When selecting a location for observing, get as far away as
possible from direct artificial light such as street lights, porch
lights, and automobile headlights. The glare from these lights
will greatly impair your dark‑adapted night vision. Set up on
a grass or dirt surface, not asphalt, because asphalt radiates
more heat. Heat disturbs the surrounding air and degrades
the images seen through the telescope. Avoid viewing over
rooftops and chimneys, as they often have warm air currents
rising from them. Similarly, avoid observing from indoors
through an open (or closed) window, because the tempera‑
ture difference between the indoor and outdoor air will cause
image blurring and distortion.
If at all possible, escape the light‑polluted city sky and head
for darker country skies. You’ll be amazed at how many more
stars and deep‑sky objects are visible in a dark sky!
“seeing" and transparency
Atmospheric conditions vary significantly from night to night.
“Seeing" refers to the steadiness of the Earth’s atmosphere at
a given time. In conditions of poor seeing, atmospheric turbu‑
lence causes objects viewed through the telescope to “boil".
If, when you look up at the sky with just your eyes, the stars
are twinkling noticeably, the seeing is bad and you will be lim‑
ited to viewing with low powers (bad seeing affects images at
high powers more severely). Planetary observing may also be
poor.
In conditions of good seeing, star twinkling is minimal and
images appear steady in the eyepiece. Seeing is best over‑
head, worst at the horizon. Also, seeing generally gets better
after midnight, when much of the heat absorbed by the Earth
during the day has radiated off into space.
Especially important for observing faint objects is good “trans‑
parency"—air free of moisture, smoke, and dust. All tend to
scatter light, which reduces an object’s brightness. Transparency
is judged by the magnitude of the faintest stars you can see with
the unaided eye (6th magnitude or fainter is desirable).
Atmospheric conditions vary significantly from night to night.
“Seeing" refers to the steadiness of the Earth’s atmosphere at
a given time. In conditions of poor seeing, atmospheric turbu‑
lence causes objects viewed through the telescope to “boil".
If, when you look up at the sky with just your eyes, the stars
are twinkling noticeably, the seeing is bad and you will be lim‑
ited to viewing with low powers (bad seeing affects images at
high powers more severely). Planetary observing may also be
poor.
In conditions of good seeing, star twinkling is minimal and
images appear steady in the eyepiece. Seeing is best over‑
head, worst at the horizon. Also, seeing generally gets better
after midnight, when much of the heat absorbed by the Earth
during the day has radiated off into space.
Especially important for observing faint objects is good “trans‑
parency"—air free of moisture, smoke, and dust. All tend to
scatter light, which reduces an object’s brightness. Transparency
is judged by the magnitude of the faintest stars you can see with
the unaided eye (6th magnitude or fainter is desirable).
cooling the telescope
All optical instruments need time to reach “thermal equilibri‑
um". The bigger the instrument and the larger the temperature
change, the more time is needed. Allow at least 30 minutes
for your telescope to cool to the temperature outdoors. In very
cold climates (below freezing), it is essential to store the tele‑
scope as cold as possible. If it has to adjust to more than a
40° temperature change, allow at least one hour.
All optical instruments need time to reach “thermal equilibri‑
um". The bigger the instrument and the larger the temperature
change, the more time is needed. Allow at least 30 minutes
for your telescope to cool to the temperature outdoors. In very
cold climates (below freezing), it is essential to store the tele‑
scope as cold as possible. If it has to adjust to more than a
40° temperature change, allow at least one hour.
let Your Eyes Dark‑adapt
Don’t expect to go from a lighted house into the darkness of
the outdoors at night and immediately see faint nebulas, galax‑
ies, and star clusters—or even very many stars, for that matter.
Your eyes take about 30 minutes to reach perhaps 80% of
their full dark‑adapted sensitivity. As your eyes become dark‑
Don’t expect to go from a lighted house into the darkness of
the outdoors at night and immediately see faint nebulas, galax‑
ies, and star clusters—or even very many stars, for that matter.
Your eyes take about 30 minutes to reach perhaps 80% of
their full dark‑adapted sensitivity. As your eyes become dark‑
Figure 6: This illustration shows the telescope pointed in the
four cardinal directions: (a) north, (b) south, (c) east, (d) west.
Note that the tripod and mount have not been moved; only the
telescope tube has been moved on the R.A. and Dec. axes.
four cardinal directions: (a) north, (b) south, (c) east, (d) west.
Note that the tripod and mount have not been moved; only the
telescope tube has been moved on the R.A. and Dec. axes.
a. b.
c. d.