The Sky #2 ?? Extra Credit Lab ?? 1 name TAKE HOME VERSION OF SKY-LAB #1 OR AN EXTRA CREDIT LAB THE SKY AND CONSTELLATION TOUR: 2. USING SKY CHARTS GET A COPY OF THE PRE-LAB OF THE FIRST SKY-LAB READ...

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Answered Same DayDec 21, 2021

Answer To: The Sky #2 ?? Extra Credit Lab ?? 1 name TAKE HOME VERSION OF SKY-LAB #1 OR AN EXTRA CREDIT LAB THE...

David answered on Dec 21 2021
125 Votes
Lab 3:
Solution 1:
Star Babba is closer to us as the arc shift of this star is smaller. We consider that the parallax angle
formed by each is same. Then,





A1= shift of abba
B1= shift of babba
A1>B1
Let A1=xB1 where x>
1



Hence R1>R2
Hence Babba is nearer.
Solution 2:
Arc length is given by:
Where:
A= arc length
R=radius
When star abba has twice the angle then it can be written:
Hence the distance of star Babba is twice that of star Abba.
Solution 3:
No it will not be able to detect the arc shift as the measurement using parallax is done for nearby stars.
The angle less that 0.01 sec is very difficult to measure.
Solution 4:
The sun should be located at the centre of the milky way so that it can measure stars at a range of 1300
light year . hence the at this location the fraction of milky way sun can measure is:




0.013 part of milky way can be measured.
Solution 5:
According to the given explanation it is said that if the angle of the star is ½ arc sec then the distance of
a star is 2 parasec.
This means if the angle is x arc second then the distance is 1/x para second.
Hence:




Where d=distance of the star
And p=parallax angle.
Solution 6:
Yes the graph matches the previous expression.
Angle distance
0.1 10
0.2 5
0.4 2.5
0.5 2
0.7 1.42
0.75 1.33
Solution 7:
From relation in question 5 we know that the smaller the angle larger is its distance.
Rank Star Angle
3rd Antares 0.024
1st Ross 780 0.213
2nd Regulus 0.045
4th Betelgeuse 0.009
Solution 8:
Star name Parallax Distance
Arcturus 0.09 11.11
Procyon 0.288 3.47
Hadar 0.006 166.67
Rigel 0.004 250
Sirius 0.379 2.638
Altair 0.194 5.155
Solution 9:
Since the accurate measurement can’t be made hence taking a rough view.
Angular shift:
A=0.1 arc sec B=2*0.1=0.2arc sec
Parallax gives the angular shift hence, both are same:
A=0.1 arc sec B=2*0.1=0.2arc sec
Distance of each star in para sec is:








Solution 10:
The result in question 9 can have an uncertainty of 10 to 20%. Since there is no bottom scale provided
hence using a random scale it is measured.
The distance calculated for long distance star is based on the parallax the form at two different time’s.
This distance is measured over a time of several months hence a small difference...
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