Meade 114 EQ-D Understanding Celestial Movements and Coordinates, Celestial Sphere

– 8 –

•Unlock the R.A. lock (22, Fig. 1) and the Dec. lock (23, Fig. 1) so that the telescope turns freely on both axes. Then point the main telescope at some well-defined land object (e.g. the top of a telephone pole) at least 200 yards distant, and re-lock the R.A and Dec. axes. Turn the flexible cable controls, (3, Fig. 1) and (4, Fig. 1), to center the object in the telescopic field.

•With the front of the viewfinder already centered in the front bracket ring, look through the viewfinder and loosen or tighten, as appropriate, one or more of the rear viewfinder bracket ring thumbscrews (26, Fig. 1) until the viewfinder’s crosshairs are likewise centered on the object previously centered in the main telescope.

•Check this alignment on a celestial object, such as a bright star or the Moon, and make any refinements necessary, using the method outlined above.

With this alignment performed, objects first located in the wide-field viewfinder will also be centered in the main telescope’s field of view. (Note: The viewfinder presents an image which is upside-down.)

UNDERSTANDING CELESTIAL MOVEMENTS AND COORDINATES

Understanding where to locate celestial objects, and how those objects move across the sky is fundamental to enjoying the hobby of astronomy. Most amateur astronomers adopt the simple practice of “star-hopping” to locate celestial objects by using star charts or astronomical software which identify bright stars and star patterns (constellations) that serve as “road maps” and “landmarks” in the sky. These visual reference points guide amateur astronomers in their search for astronomical objects. And, while star-hopping is the preferred technique, a discussion of using setting circles for locating objects is desirable since your telescope is provided with this feature. However, be advised, compared to star hopping, object location by use of setting circles requires a greater investment in time and patience to achieve a more precise alignment of the telescope’s polar axis to the celestial pole. For this reason, in part, star-hopping is popular because it is the faster, easier way to become initiated in the hobby.

Understanding how astronomical objects move: Due to the Earth’s rotation, celestial bodies appear to move from East to West in a curved path through the skies. The path they follow is known as their line of Right Ascension (R.A.). The angle of this path they follow is known as their line of Declination (Dec.). Right Ascension and Declination is analogous to the Earth-based coordinate system of latitude and longitude.

Understanding celestial coordinates: Celestial objects are mapped according to the R.A. and Dec. coordinate system on the “celestial sphere” (Fig. 2), the imaginary sphere on which all stars appear to be placed. The Poles of the celestial coordinate system are defined as those 2 points where the Earth's rotational axis, if extended to infinity, North and South, intersect the celestial sphere. Thus, the North Celestial Pole is that point in the sky where an extension of the Earth's axis through the North Pole intersects the celestial sphere. In fact, this point in the sky is located near the North Star, or Polaris.

On the surface of the Earth, “lines of longitude” are drawn between the North and South Poles. Similarly, “lines of latitude” are drawn in an East-West direction, parallel to the Earth's equator. The

celestial

equator

is

simply

a

projection of the Earth's equator

+90° Dec.

North Celestial Pole

onto the celestial sphere. Just as on

(Vicinity of Polaris)

Star

the surface of the Earth, imaginary

lines have been

drawn on

the

D

é

c

l

i

celestial

sphere

to

form

a

n

a

i

s

13

12

11

o

coordinate

grid. Celestial object

15

14

10

n

9

17

16

8

7

positions on the Earth's surface are

18

Rotation de la Terre

6

19

4

5

specified

by

their

latitude

and

20

3

21

22 23

2

0

1

0° Déc.

Celestial

longitude.

Ascension droite

Equator

The celestial equivalent to Earth

latitude is

called

“Declination,”

or

South

simply “Dec,”

and

is measured

in

Celestial .

-90° Dec.

degrees,

minutes

and

seconds

Pole

north ("+") or south ("-") of the

celestial equator. Thus any point on

Fig. 2: Celestial Sphere.