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Observing Stellar Heartbeats

Look at the simulated reproduction of a star field below. It contains a variable star that is located in the middle of a set of crosshairs, and surrounding the variable star are several comparison stars of known magnitudes. These stars, which do not vary in brightness, are used to compare the changing brightness, or magnitude, of the variable star. Knowing the values of the magnitudes of the comparison stars, you can estimate the magnitude of the variable star as it changes over time. On a star chart, different magnitudes are portrayed as different sizes - the brighter the magnitude the larger the size of the star, and the dimmer the magnitude the smaller the size of the star. Magnitudes have one decimal, such as 6.3 - however in star fields, the decimals are not indicated. A magnitude of 6.3 is written as 63 so that the fields are not as cluttered and the decimal points are not mistaken for stars. When you record your magnitude estimation you need to include the decimal.

Julian Date Slide Show

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Print out the table provided. Estimate the magnitude of the variable star on the first picture of the star field using the magnitudes of the stars around it. Proceed through each of the pictures and place your estimated magnitudes and the corresponding Julian Day (JD) numbers in the table.

Ask your students to look closely at the first plate. Question them about what they see in each plate. Suggestions are:
  1. How is the target variable star marked? (with crosshairs)
  2. How are comparison star magnitudes designated? (Emphasize the backward-nature stellar magnitude. Brighter stars are indicated with large dots and a SMALL number, dimmer stars with smaller dots and larger numbers. A useful analogy is 1st place, 2nd place, as in a race.)
  3. Is there a star of magnitude 5.7? What do you notice about it's representation? (The magnitude is written as 57, so that decimal points are not confused with stars.)
  4. Look at the JD numbers below the plate. What do you notice about the numbers (The dates are sequential and part of the number, "2449", is repetitive. Plates can be uniquely identified with only the last three numerals.)
  5. Does the target variable star have the same magnitude on any of the plates (Yes, look at JD +300 and JD +435.)


Next: Recording Stellar Heartbeats

Return to Variable Stars Index


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