Celestial and Horizon Coordinate Systems
How do astronomers say exactly where an object is in the sky? Learn the two coordinate systems - equatorial and horizon - the key terms, and how the altitude of Polaris reveals your latitude.
Work through it, step by step
Work through it free and interactively, with each step checked before the next.
Start revising freeWhat you'll cover
Pinning down a point in the sky
To say exactly where a star is, astronomers imagine the sky as a giant celestial sphere around Earth, with celestial poles above Earth's poles and a celestial equator above the equator. There are two ways to give a position on it: the equatorial system (fixed to the stars) and the horizon system (what you actually see from your spot right now). This module covers both, the key terms, and how the sky reveals your latitude.
Words for the sky
These terms describe where things are and how they move. Learn them - the next steps use them.
Zenith, meridian, culmination
- Zenith
- Meridian
- Culmination
- Diurnal motion
- The point directly above the observer
- The north-south line through the zenith
- A star crossing the meridian at its highest point
- The daily east-to-west apparent motion of the sky
Which term is this?
You look at the exact point in the sky directly above your head. What is that point called?
- The zenith
- The meridian
- The celestial pole
- The horizon
Two coordinate systems
Both give a position with two numbers, but they answer different questions. One is fixed to the stars; one describes your personal view right now.
Match each coordinate to what it measures
- Right ascension
- Declination
- Altitude
- Azimuth
- Position around the celestial equator, like longitude
- Angle north or south of the celestial equator
- Angle of an object above the horizon
- Angle measured around the horizon from north
Fixed to the stars?
A star chart lists an object's position so that any observer, anywhere, can find it. Which coordinate system does a star chart use?
- Equatorial (right ascension and declination), fixed to the stars
- Horizon (altitude and azimuth)
- Just the cardinal points (N, E, S, W)
- Altitude on its own
What the pole tells you
Two rules the exam loves:\n\n- The altitude of the celestial pole equals your latitude. In the north, Polaris sits almost exactly at the pole, so the altitude of Polaris is your latitude. Measure it and you know how far north you are. - A star is circumpolar (never sets) if its declination is greater than 90 minus your latitude. The nearer you are to a pole, the more of the sky circles overhead and never dips below the horizon.
Find the latitude
An observer in the northern hemisphere measures Polaris at an altitude of 51 degrees above the horizon. What is the observer's latitude, in degrees north?
What is true up there?
Select the TWO statements that are correct.
- The altitude of the celestial pole equals the observer's latitude
- A circumpolar star never sets below the horizon
- Right ascension is measured in metres
- Azimuth is the angle of an object above the horizon
A star across the night
Put the stages of a (non-circumpolar) star's nightly path across the sky into order.
- The star rises above the eastern horizon
- It climbs higher into the sky
- It reaches its highest point as it crosses the meridian (culmination)
- It descends towards the west
- It sets below the western horizon
Which system, which star?
Three quick decisions about coordinates and circumpolarity.
- At latitude 51 degrees north, a star is circumpolar if its declination is above 39 degrees (90 - 51). A star has declination 60 degrees. Is it circumpolar there?
- You want to record a star's position so an observer on the other side of the world can find it too. Which system do you use?
- You want to tell a friend standing next to you exactly where to point their telescope right now. Which system is most practical?
Equatorial or horizon?
Explain the difference between the equatorial and horizon coordinate systems, and describe how the altitude of Polaris lets an observer work out their latitude.
- Name the two coordinates in each system (RA and declination; altitude and azimuth)
- Explain why equatorial coordinates are fixed to the stars while horizon coordinates depend on place and time
- State the rule that the altitude of the celestial pole equals the observer's latitude
- Give a worked example (for example Polaris at altitude 51 degrees means latitude 51 degrees north)
Altitude equals latitude
Two rules unlock most of the marks in this topic. First, the altitude of the pole equals your latitude - so the altitude of Polaris IS your latitude in the north. Learn it and the calculations fall out. Second, circumpolar means declination greater than 90 minus latitude. Beyond that, always pick the right system for the job: equatorial (RA and dec) when the position must be the same for everyone, horizon (altitude and azimuth) when you are pointing at the sky here and now.