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מצפה הכוכבים ברקת - קוד מצפה רשמי Bareket observatory IAU B35

לחיפוש במונחון הזן טקסט ולחץ חפש


מנוח הסבר המונח
Absolute Magnitude

A scale for measuring the actual brightness of a celestial object. Absolute magnitude measures how bright an object would appear if it were exactly 10 parsecs (about 33 light years) away from Earth.

Angular resolution

The ability of an instrument such as a telescope, to distinguish objects that are close to each other. The angular resolution of an instrument is the smallest angular separation at which the instrument can observe two neighboring objects as two separate objects. The angular resolution of the human eye is about a minute of arc, while it can get up to 0.7' arc min for people with an extreamly good eyesight.

Angular Size

The apparent size of an object in the sky, or the distance between two objects, measured as an angle. Your index finger held at arm’s length spans about 1°, your fist about 10°. 

מפתח הטלסקופ. ראה הרחבה במאמר לבחירת טלסקופ.

The diameter of a telescope’s main lens or mirror — and the scope’s most important attribute. As a rule of thumb, a telescope’s maximum useful magnification is 50 times its aperture in inches (or twice its aperture in millimeters).


The point in its orbit where a planet is farthest from the Sun.


The point in the orbit of the moon or a satellite, at which it is furthest from the Earth


perigee versus apogee

Illustration: perigee ‘Supermoon’ versus an apogee ‘Minimoon’

Apparent Magnitude

The apparent brightness of an object in the sky as it appears to an observer on Earth.

Arc minute

One arc minute is 1/60 of a degree of arc. The angular diameter of the full moon or the Sun as seen from Earth is about 30 arc minutes - 1/2 arc degree.

Arc second

One arc second is 1/60 of an arc minute = 1/3600 of an arc degree. The angular diameter of Jupiter varies from about 30 to 50 arc seconds, depending on its distance from Earth.


A small planetary body in orbit around the Sun. Smaller than a planet. Most asteroids can be found in a belt between the orbits of Mars and Jupiter. The orbits of some asteroids take them close to the Sun, which also takes them across the paths of the planets.

Asteroid belt

A region of space between Mars and Jupiter where the great majority of asteroids is found

Astro EDU network

The Astro-Edu-Net initiative provides a number of fascinating resources for astronomy and space, including access to virtual and remote robotic telescopes, as well as interactive applications.

With them, students can explore mathematics, physics, geography and other subjects using genuine astronomy and space-related data, and making real scientific observations.

The Astro-Edu is has been conducted by the Bareket observatory.


A scientist who studies the universe and the celestial bodies residing in it, including their composition, history, location, and motion.

Astronomical unit

The average distance from the Earth to the Sun; 1 AU is ~149,597,900 kilometers (~92,960,120 miles).


The layer of gases surrounding the surface of a planet, moon, or star

Big Bang

A broadly accepted theory for the origin and evolution of our universe. The theory says that the observable universe started roughly 13.7 billion years ago from an extremely dense and incredibly hot initial state.

Binary Stars

System of two stars that revolve around a common center of gravity.

Black Hole

Stars that are very massive will collapse under their own gravity when their fuel is exhausted. The collapse continues until all matter is 'crushed' into what is known as a singularity. The gravitational pull of a black hole is so strong that from a certain distance not even light can escape.


An exploding meteorite

Cassegrain telescope

A type of reflecting telescope whose eyepiece is located behind the primary mirror. The primary mirror is cast with a hole in the center. When light enters the telescope, it reflects from the primary mirror to the secondary mirror. The secondary mirror reflects the light back through the hole in the primary mirror to the eyepiece.