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Equatorial Alignment
In equatorial (or “polar”) Alignment, the telescope is oriented so that the horizontal
and vertical axes of the telescope are lined up with the celestial coordinate system.
In order to equatorial align your telescope, it is essential to have an understanding of
how and where to locate celestial objects as they move across the sky. This section
provides a basic introduction to the terminology of equatorial-aligned astronomy, and
includes instructions for finding the celestial pole and for finding objects in the night
sky using Declination and Right Ascension.
Celestial Coordinates
A celestial coordinate system was created that maps an imaginary sphere
surrounding the Earth upon which all stars appear to be placed. 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 and
longitude grid for 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 poles of this coordinate system are defined as those two points where the Earth’s
North and South poles (
i.e.,
the Earth’s axis), if extended to infinity, would cross the
celestial sphere. Thus, the North Celestial Pole (Fig. 38, 1) is that point in the sky
where an extension of the North Pole intersects the celestial sphere. The North Star,
Polaris, is located very near the North Celestial Pole (Fig. 38, 1). The celestial equator
(Fig. 38, 2) is a projection of the Earth’s equator onto the celestial sphere.
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 could locate Los Angeles, California, by its latitude
(+34°) and longitude (118°). Similarly, you could locate the Ring Nebula (M57) by its
Right Ascension (18hr) and its Declination (+33°).
W
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
arbitrarily 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.
W
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°). Dec. locations South of the celestial equator are indicated with a
minus (–) sign (
e.g.
, the Dec. of the South celestial pole is –90°). Any point on
the celestial equator (such as the the constellations of Orion, Virgo, and
Aquarius) is said to have a Declination of zero, shown as 0° 0' 0".
Setting Circles
Setting circles included with the
LX200-ACF
models permit the location of faint
celestial objects not easily found by direct visual observation. The R.A. circle (Pg. 7,
Fig. 1, 11 and Fig. 38) is located on the top surface of the telescope’s drive base. The
Declination circle (Fig. 37) is located at the top of the fork tine. With the telescope
pointed at the North Celestial Pole, the Dec. circle should read 90° (understood to
mean +90°). Objects located below the 0-0 line of the Dec. circle carry minus
Declination coordinates. Each division of the Dec. circle represents a 1° increment.
The R.A. circle runs from 0
hr
to (but not including) 24
hr
, and reads in increments of 5
min
.
Fig. 36: Celestial Sphere.
APPENDIX A: EQUAT O R I A L
(POLAR) ALIGNMENT
Important Note:
The “Telescope: Mount”option
of the Setup menu is set to
“Alt/Az” as the default mount
by the factory. The example
presented in this section
assumes that you are
performing an alignment
procedure for the first time
with your telescope and
therefore, the “Te l e s c o p e :
Mount” option does not need
to be selected.
If the telescope is equatorially
mounted, you must choose
the “Polar” option from the
AutoStar II “Telescope Mount”
m e n u .
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