Meade polaris 90 мм Инструкция по эксплуатации онлайн [10/28] 159829
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and longitude on the celestial sphere. These
lines are known as Right Ascension and
Declination.
The celestial map also contains two poles
and an equator just like a map of the Earth.
The celestial poles are defined as those two
points where the Earth’s North and South
poles, if extended to infinity, would cross the
celestial sphere. Thus, the North Celestial
Pole is that point in the sky where the North
Pole crosses the celestial sphere. The North
Star, Polaris, is located very near the North
Celestial Pole.
So, just as an object’s position on the
Earth’s surface can be located by its latitude
and longitude, celestial objects may also
be located using Right Ascension and
Declination. For example: You can locate
Los Angeles, California, by its latitude
(+34°) and longitude (118°). Similarly, you
can locate the Ring Nebula (also known as
“M57”) by its Right Ascension (18hr) and its
Declination (+33°).
• RIGHT ASCENSION (R.A.): This Celestial
version of longitude is measured in units of
hours (hr), minutes (min), and seconds (sec)
on a 24 hour “clock” (similar to how Earth’s
time zones are determined by longitude lines).
The “zero” line was chosen to pass through
the constellation Pegasus, a sort of cosmic
Greenwich meridian. R.A. coordinates range
from 0hr 0min 0sec to 23hr 59min 59sec.
There are 24 primary lines of R.A., located
at 15-degree intervals along the celestial
equator. Objects located further and further
East of the zero R.A. grid line (0hr 0min 0sec)
carry higher R.A. coordinates.
• Declination (Dec.): This celestial version
of latitude is measured in degrees, arc-
minutes, and arc-seconds (e.g., 15° 27’ 33”).
Dec. locations North of the celestial equator
are indicated with a plus (+) sign (e.g., the
Dec. of the North celestial pole is +90°). Any
point on the celestial equator (such as the
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Earth. This mapping system is similar to
the system of latitude and longitude on
Earth surface maps.
In mapping the surface of the Earth,
lines of longitude are drawn between the
North and South Poles and lines of latitude
are drawn in an East-West direction, parallel
to the Earth’s equator. Similarly, imaginary
lines have been drawn to form a latitude
Fig. 7
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1
12
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Rotation
of the
Earth
0 Dec.
South
Celestial
Pole
Right
Ascension
Star
Celestial
Equator
-90 Dec.
+90 Déc.
D
e
c
l
i
n
a
t
i
o
n
North
Celestial
Pole
(Vicinity of
Polaris)
Looking at or near the Sun will cause irreversable damage to your eye. Do not point this telescope at or near the Sun. Do not look through the telescope as it is moving.
8
Содержание
- Meade instruction manual 1
- Polaris series 1
- Warning 2
- Figure 1a 4
- Figure 1a meade polaris reflecting telescope inset a accessory tray 4
- Inset a 4
- Inset b 4
- Inset b inset b red dot viewfinder assembly 4
- Inset c 4
- Inset c inset c tripod leg 4
- Figure 1b 5
- Figure 1b meade polaris refracting telescope inset a accessory tray 5
- Inset a 5
- Inset b 5
- Inset b inset b red dot viewfinder assembly 5
- Inset c 5
- Inset c inset c tripod leg 5
- Replace with english text 19
- A correct collimation 21
- All meade polaris reflecting telescopes are optically aligned at the factory prior to shipment it is unlikely that you will need to align or collimate the optics after receipt of the instrument however if the telescope received unusually rough handling in 21
- Collimation alignment of optics reflecting models only 21
- Fig 13 21
- Fig 14 21
- Fig 15 21
- Fig 16 21
- Fig 17 21
- Shipment it is possible that the optics must be re aligned for best optical performance in any case this alignment procedure is simple and requires only a few minutes the very first time the telescope is used take the time to familiarize yourself with the following collimation procedure so that 21
- The properly collimated aligned mirror system in the meade polaris telescope assures the sharpest images possible this occurs when the primary mirror and secondary mirror are tilted so that the focused image falls directly through the center of the focuser draw tube these mirror tilt adjustments are made with the secondary mirror assembly and the primary mirror cell fig 13 and will be discussed later 21
- Tissues or damage could result to the optics do not use a commercial photographic lens cleaner 21
- You will recognize a properly collimated instrument and can adjust the collimation yourself if necessary 21
- Push here to open battery compartment 24
- Www meade com 28
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