Software specifications, Appendix b - glossary of terms – Celestron CPC Deluxe 1100 HD Computerized Telescope User Manual

Page 36

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Software Specifications

Ports

RS-232 communication port on hand control, Autoguider Port, 2 Auxiliary Port, PC Port

Period Error Correction

Permanently programmable

Tracking Rates

Sidereal, Solar, Lunar

Tracking Modes

Alt-Az, EQ North and EQ South

Alignment Procedures

Sky Align, Auto Two-Star Align, Two-Star Align, Solar System Align, EQ North Align

and EQ South Align

Database

40,000+ objects, 99 user defined programmable objects.

Enhanced information on over 200 objects

Complete Revised NGC Catalog

7,840

Complete Messier Catalog

110

Complete IC Catalog

5,386

Complete Caldwell

109

Abell Galaxies

2,712

Solar System objects

9

Famous Asterisms

20

Selected CCD Imaging Objects

25

Selected SAO Stars

29,500

APPENDIX B - GLOSSARY OF TERMS

A –

Absolute

The apparent magnitude that a star

magnitude

would have if it were observed from a

standard distance of 10 parsecs, or 32.6 light–

years . The absolute magnitude of the Sun is

4.8. at a distance of 10 parsecs, it would just

be visible on Earth on a clear moonless night

away from surface light .

Airy disk

The apparent size of a star’s disk produced even by
a perfect optical system . Since the star can never
be focused perfectly, 84 per cent of the light will
concentrate into a single disk, and 16 per cent into a
system of surrounding rings .

Alt–Azimuth

A telescope mounting using two

Mounting

independent rotation axes allowing

movement of the instrument in Altitude

and Azimuth .

Altitude

In astronomy, the altitude of a celestial object is
its Angular Distance above or below the celestial
horizon .

Aperture

The diameter of a telescope’s primary lens or mirror;
the larger the aperture, the greater the telescope’s
light–gathering power.

Apparent

A measure of the relative brightness of a

Magnitude

star or other celestial object as perceived

by an observer on Earth .

Arc minute

A unit of angular size equal to 1/60 of
a degree .

Arc second

A unit of angular size equal to 1/3,600 of a degree (or
1/60 of an arc minute).

Asterism

A small unofficial grouping of stars in the
night sky .

Asteroid

A small, rocky body that orbits a star .

Astrology

The pseudoscientific belief that the positions of stars

and planets exert an influence on human affairs;
astrology has nothing in common with astronomy .

Astronomical

The distance between the Earth and the Sun .

unit (AU)

It is equal to 149,597,900 km., usually

rounded off to 150,000,000 km.

Aurora

The emission of light when charged particles from
the solar wind slams into and excites atoms and
molecules in a planet’s
upper atmosphere .

Azimuth

The angular distance of an object eastwards along
the horizon, measured from due north, between
the astronomical meridian (the vertical line passing
through the center of the sky and the north and
south points on the horizon) and the vertical line
containing the celestial body whose position is to
be measured .

B –

Binary Stars

Binary (Double) stars are pairs of stars that, because
of their mutual gravitational attraction, orbit around
a common center of mass. If a group of three or
more stars revolve around one another, it is called
a multiple system. It is believed that approximately
50 percent of all stars belong to binary or multiple
systems . Systems with individual components that
can be seen separately by a telescope are called
visual binaries or visual multiples . The nearest “star”
to our solar system, Alpha Centauri, is actually our
nearest example of a multiple star system. It consists
of three stars, two very similar to our Sun and one
dim, small, red star orbiting around one another .

C –

Celestial

The projection of the Earth’s equator

Equator

on to the celestial sphere. It divides the sky

into two equal hemispheres .

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