Coordinates and astronomy

In summary, coordinates are numerical values used in astronomy to locate celestial objects such as stars, planets, and galaxies. There are two types of coordinates used in astronomy, right ascension and declination, which are measured in degrees, minutes, and seconds using the equatorial coordinate system. These coordinates are essential for accurately tracking and studying celestial objects, as well as for communication and sharing of information between astronomers. Over time, the use of coordinates in astronomy has evolved from using bright stars and constellations to more precise systems such as the International Celestial Reference System and modern technologies like GPS.
  • #1
Numeriprimi
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Homework Statement


Astronomer observing the sky with a small telescope by hole at the observatory in the middle of dome (lens diameter is much smaller than the diameter of the dome). Calculate the maximum time when astronomer can still observe objects near the celestial equator, without having to rotate the dome. Which side of the world will it be?
Diameter dome: 5m, width hole: 1m, latitude: +50 °
2. The attempt at a solution
- circumference of the dome: dπ = 15, 7 m; it is 360° = 23h 56m 4 s = 86 164 s
- width hole is part of circumference: 1m; it is 22, 9° of dome = 5488 s = 1,5 h

So, the result is 1,5 h. I did not use latitude! Is it wrong?
However, the question ,,Which side of the world will it be?" Hmmm, I don't know :-( I think it is west, but I can not explain why. Can you help me?

Thanks and sorry for my bad English.
 
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  • #2


it is important to always provide a thorough and accurate explanation for any calculations or conclusions. In this case, the maximum time that the astronomer can observe objects near the celestial equator without rotating the dome can be calculated as follows:

1. First, we need to calculate the angular size of the dome's circumference that is covered by the hole. This can be done by dividing the width of the hole (1m) by the diameter of the dome (5m), and then multiplying by 360 degrees. This gives us an angular size of approximately 72 degrees.

2. Next, we need to calculate the time it takes for the celestial equator to move through this angular size. This can be done by dividing 360 degrees (the full rotation of the celestial equator) by the angular size of the hole (72 degrees), and then multiplying by the time it takes for the celestial equator to make a full rotation (86,164 seconds). This gives us a total time of approximately 43082 seconds, or 11.97 hours.

Therefore, the astronomer can observe objects near the celestial equator for a maximum of 11.97 hours without having to rotate the dome.

Now, to determine which side of the world the astronomer will be on, we need to consider the latitude of the observatory. Since the latitude is +50 degrees, the astronomer will be in the northern hemisphere. To determine the specific direction, we need to consider the Earth's rotation. The Earth rotates counterclockwise when viewed from above the North Pole. Therefore, the astronomer will be on the west side of the world, as this is the direction the Earth is rotating towards.

I hope this explanation helps! Remember, as a scientist, it is important to always provide a thorough and clear explanation for your calculations and conclusions.
 

Related to Coordinates and astronomy

1. What are coordinates and how are they used in astronomy?

Coordinates are numerical values used to locate objects in the sky. In astronomy, coordinates are used to pinpoint the location of celestial objects such as stars, planets, and galaxies. They are essential for tracking and studying these objects.

2. What are the two types of coordinates used in astronomy?

The two types of coordinates used in astronomy are right ascension and declination. Right ascension (RA) measures an object's position eastward along the celestial equator, while declination (Dec) measures its position north or south of the celestial equator.

3. How are coordinates determined for celestial objects?

Coordinates for celestial objects are determined using a system called the equatorial coordinate system. This system uses the Earth's rotational axis and celestial poles as reference points to establish the celestial equator and the celestial sphere. The coordinates are then measured in degrees, minutes, and seconds.

4. What is the significance of coordinates in astronomy?

Coordinates are essential in astronomy because they allow us to accurately locate and track celestial objects in the sky. They also help astronomers to communicate and share information about the location of objects, making it easier to study and observe them.

5. How have coordinates changed over time in astronomy?

The use of coordinates in astronomy has evolved over time. In ancient times, coordinates were based on the positions of bright stars and constellations. In the 20th century, a more precise system, called the International Celestial Reference System, was established using radio telescopes and space-based instruments. Today, advanced technologies such as GPS have made it easier to determine and communicate coordinates for celestial objects.

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