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GCSE Astronomy Help plsssssss

Someone please explain all the stuff in the parts of celestial observations below:
6.8 Understand the use of the equatorial coordinate system
(right ascension and declination)
5a, 5b, 5c
6.9 Understand the use of the horizon coordinate system
(altitude and azimuth)
5a, 5b, 5c
6.10 Understand how the observer’s latitude can be used to link the
equatorial and horizon coordinates of an object for the
observer’s meridian
1a
4a
5a, 5b, 5c
6.11 Understand how the observer’s meridian defines local sidereal
time and an object’s hour angle
1a
4a
5a, 5b, 5c
6.12 Be able to use information on equatorial and horizon
coordinates to determine:
a the best time to observe a particular celestial object
b the best object(s) to observe at a particular time
1a
4a
5a, 5b, 5c
Thanks in advance!!

Reply 1

Original post
by koalasarethebest
Someone please explain all the stuff in the parts of celestial observations below:
6.8 Understand the use of the equatorial coordinate system
(right ascension and declination)
5a, 5b, 5c
6.9 Understand the use of the horizon coordinate system
(altitude and azimuth)
5a, 5b, 5c
6.10 Understand how the observer’s latitude can be used to link the
equatorial and horizon coordinates of an object for the
observer’s meridian
1a
4a
5a, 5b, 5c
6.11 Understand how the observer’s meridian defines local sidereal
time and an object’s hour angle
1a
4a
5a, 5b, 5c
6.12 Be able to use information on equatorial and horizon
coordinates to determine:
a the best time to observe a particular celestial object
b the best object(s) to observe at a particular time
1a
4a
5a, 5b, 5c
Thanks in advance!!

Hey! This seems like a pretty detailed set of concepts related to celestial observations, but I’ll break it down for you as simply as possible.

1.

Equatorial Coordinate System (Right Ascension and Declination): Think of this as the celestial equivalent of longitude and latitude, but for stars and celestial objects.

2.

Right Ascension is like longitude but for the sky. It’s measured in hours, minutes, and seconds.

3.

Declination is like latitude, measuring how far above or below the celestial equator an object is.

4.

Horizon Coordinate System (Altitude and Azimuth): This system is based on the observer’s location and the horizon.

5.

Altitude refers to how high up an object is in the sky (0° is at the horizon, 90° is directly overhead).

6.

Azimuth is the angle of the object in the sky, measured from the north, going east (0° is north, 90° is east, etc.).

7.

Linking Equatorial and Horizon Coordinates with Latitude: Your latitude can help you convert between equatorial and horizon coordinates. This is because where you are on Earth affects how you see the sky.

8.

Meridian and Local Sidereal Time: The observer’s meridian is an imaginary line running from north to south through your location. It helps you track local sidereal time, which is like the time for the stars, and also tells you the hour angle of an object—how far along its path it is relative to the observer's meridian.

Using Coordinates to Determine the Best Time/Objects to Observe: By understanding both equatorial and horizon coordinates, you can figure out when to observe a particular celestial object or which objects are best to observe at a given time.

Reply 2

Original post
by Toptutor_richard
Hey! This seems like a pretty detailed set of concepts related to celestial observations, but I’ll break it down for you as simply as possible.

1.

Equatorial Coordinate System (Right Ascension and Declination): Think of this as the celestial equivalent of longitude and latitude, but for stars and celestial objects.

2.

Right Ascension is like longitude but for the sky. It’s measured in hours, minutes, and seconds.

3.

Declination is like latitude, measuring how far above or below the celestial equator an object is.

4.

Horizon Coordinate System (Altitude and Azimuth): This system is based on the observer’s location and the horizon.

5.

Altitude refers to how high up an object is in the sky (0° is at the horizon, 90° is directly overhead).

6.

Azimuth is the angle of the object in the sky, measured from the north, going east (0° is north, 90° is east, etc.).

7.

Linking Equatorial and Horizon Coordinates with Latitude: Your latitude can help you convert between equatorial and horizon coordinates. This is because where you are on Earth affects how you see the sky.

8.

Meridian and Local Sidereal Time: The observer’s meridian is an imaginary line running from north to south through your location. It helps you track local sidereal time, which is like the time for the stars, and also tells you the hour angle of an object—how far along its path it is relative to the observer's meridian.

Using Coordinates to Determine the Best Time/Objects to Observe: By understanding both equatorial and horizon coordinates, you can figure out when to observe a particular celestial object or which objects are best to observe at a given time.

I know all of this but then I see q9 on 2019 paper and i have no idea how to do it (except part c). Sry can't copy paste it cos the pdfs being annoying.

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