Sloan Digital Sky Survey
SkyServer DR14  
Not logged in Login Help

DR14 Help
 Start Here
 Cooking with Sloan
     - General
     - Solar System
     - Stars
     - Galaxies
     - QSOs/Cosmology
     - Teaching/Labs
 Contact Help Desk
 Searching SDSS
 SQL Tutorial
 SQL in SkyServer
 Sample SQL Queries
 Query Limits
 Searching Advice
 About the Database
 Table Descriptions
 Schema Browser
Create a Hubble Diagram

Back to Teaching/Labs index

Find galaxy clusters (open Famous Places in new window)

  1. The first step to create a Hubble Diagram is to find distances to galaxies. This is by far the hardest step. One simple way to do it is to use magnitudes and assume that a brighter galaxy is closer. However, this is not a safe assumption, because galaxies have different intrinsic properties – a brighter galaxy might be intrinsically brighter, but farther away.

  2. One way to get around this difficulty is to look at galaxy clusters. All the galaxies in a cluster can be assumed to be the same distance from Earth, so differences among the cluster galaxies should arise only from intrinsic differences. This means that, for example, the 5th brightest galaxy in a cluster should be just as intrinsically bright as the 5th brightest galaxy in another cluster. Therefore, observed differences in magnitudes between the 5th brightest galaxies should be due entirely to the differing distances between the clusters. This is only an approximation, but it should be enough to demonstrate the expansion of the universe.

  3. The first step, then, is to find galaxy clusters. SkyServer has a list of Abell clusters that overlap with the SDSS survey region. To download the list, click on Tools on the menu bar, then on Famous Places (link opens in new window).

  4. Scroll to the bottom of the page and click on the Abell link. You will see images of six Abell clusters, as seen by the SDSS. Scroll to the bottom of the page and click on the Abell Data link to download a CSV (comma-separated value) file containing numbers and positions (RA and dec) of Abell clusters. Save this file to your computer.

  5. Open the file with a graphing program. The SkyServer Projects provide instructions for Excel because it is a commonly used tool, but you should use whatever package you feel comfortable with.

  6. Choose a cluster you would like to study and record its RA and Dec. Repeat the next few steps for several clusters (at least 5-10).

Next: Study one cluster

Go to the previous page Go to the next page

Back to Cooking with Sloan main page
Back to Help main page
Contact Help Desk