SDSS used thousands of alumminum plates, just like the one your class has, to measure the spectrum of objects in the sky. Each hole on the plate represents the position of an object on the sky. SDSS astronomers measured the spectrum of many millions of objects: some are stars, some are galaxies and some are quasars.
Your plate has around 1000 holes in it (yes, really!), each corresponding to an object in the sky. Although all of these objects are bright enough to be seen using the SDSS telescope, you wouldn’t be able to see these with your naked eye – the constellations you are about to make were not within the reach of ancient cultures.
Step 1 – finding the brightest objects on your plate
In the same way that our ancestors chose the brightest objects in the sky to make pictures, we will choose the brightest objects in your plate. SDSS astronomers measured the magnitude of all objects in your plate, and have stored all of those numbers in a large set of tables, called a database. You will use a simple computer language called SQL to ask the database a question: which objects on my plate are the 20 brightest?
The following text does exactly that. Copy the text below, and paste it in the “SQL Search” window further down in this page:
select top 20 spa.ra, spa.dec, spa.dered_r as magnitude, spa.class, spa.z, soa.xfocal as x, soa.yfocal as yfrom specphotoAll as spajoin specObjAll as soa on soa.specObjID = spa.specObjIDwhere spa.plate = XXXXand spa.dered_r > 0order by spa.dered_r asc
Before you hit “Submit”, you will need to replace XXXX by the number of your plate. For example, if your plate is plate number 7616, then your query will look like
select top 20 spa.ra, spa.dec, spa.dered_r as magnitude, spa.class, spa.z, soa.xfocal as x, soa.yfocal as yfrom specphotoAll as spajoin specObjAll as soa on soa.specObjID = spa.specObjIDwhere spa.plate = 7616and spa.dered_r > 0order by spa.dered_r asc
When you’re ready, click “Submit”. The results will appear on the right-hand side. Then click “Download” to download your results to your local computer as a .csv file.
Step 2 – Drawing your constellation
Next, we will use a spreadsheet to plot the positions of the 20 brightest objects of your plate. The example used here is done in Google Sheets, which requires a free Goggle Account, but you can use MS Excel, or any other spreadsheet software available to you.
Create a new Sheet, and import the csv file that you downloaded from this page (File->Import). You should see your data neatly arranged in a table. Select the last two columns (X and Y) and create a “Scatter Plot”. X and Y are the coordinates of the positions of each object on the plate, with the origin being located at the centre of the plate. You should get a plot like the one shown below.
Print the scatter graph you have created. Now, in groups or individually, imagine the points in your graph are stars on the sky, and imagine what they might represent. Draw your constellation, and write a short paragraph about what it means.
Step 3 – Showing your constellation on your plate
Finally, you will light up the stars of your constellation in your plate. The X and Y positions that you used are given in millimetres, and the centre of the plate corresponds to X=0 and Y=0. With the tab of the plate pointing up, X increases to the right and Y increases down the way (moving away from the tab). Using rulers and guidelines, find the wholes that correspond to the 20 holes that you used for your constellation.
How you light up your constellation is up to you! You can use Christmas lights, or bright reflecting stickers, or anything else! Use different colours for the different types of objects, as given by the “CLASS” column.
Display your plate to the rest of your school, together with all the drawings that different groups or people in your class designed based on the lit-up pattern on your plate. Your display should explain to others what the plate is, what constellations are, and what the different classes of objects are. Send us a photograph of your display!
Step 4 – An extra challenge
In the same way that the stars of Orion are not all at the same distance from Earth, the objects in your plate are all at different distances. The column Z in your table is redshift, which astronomers can use to calculate the distance of an object to us. Typically you will find that objects with CLASS = star will have a redshift that is very close to zero, and sometimes negative. The brightest galaxies in your plate will typically have a redshift between 0.01 and 0.15, and bright quasars will have redshifts between 0.1 and 2.
The tables below tell you the distances that correspond to various values of redshift, in units of millions of light-years and in units of Megaparsec. One Megaparsec is the same as 3262000 light years. By looking for the closest values of redshift in the tables to the redshift of each of your objects, you can make a list of the distances to your objects.
Can you make a three-dimensional map of your constellation? You will need to get creative to find a way to display the distance to your objects – that is part of your challenge!