sally seebode science educator smuhsd. dean drumheller, steve howell, don hoard, sally seebode,...

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Sally Seebode Science Educator SMUHSD

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Page 1: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Sally SeebodeScience Educator SMUHSD

Page 2: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Page 3: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford
Page 4: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Take Data

Page 5: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Hardware: Losmandy G11 Mount Meade 8” SCT @f/6.3 SBIG Self Guided Spectrograph (SGS) ST7XME cameraSoftware: TheSky 6- accurate mount control CCDSoft –image acquisition Maxim DL –image acquisition IRAF –spectra processing

Page 6: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Raw Data Frame

Reduced Spectrum: standard methods using IRAF3800 – 4600A; 5800 – 6600A

Page 7: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

•EquivalentWidth

•Full Width Half

Max•Velocity

Minimum three students make measurements for each spectra, data averaged and plotted.

Page 8: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Equivalent Widths (eqw): the width of a standardized rectangle representing the area of the absorption line. EQW relates to the flux.

Exaggerated for emphasis

Page 9: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Full Width Half Max (FWHM): the width of the absorption line at half it’s maximum value. Changes in FWHM indicate velocity variations which relates to the temperature and composition of disk.

Page 10: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Velocity: Measure the central wavelength to determine if object is moving toward or away from you and at what relative velocity.

Page 11: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Small portion of data.

Page 12: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

“If I knew what I was looking for this would be much easier.”

Page 13: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Student motivation more important than math/science literacy

IRAF hard to get on high school computers

Teacher collaboration helpful Lots of support for astronomy education: NITARP, AAVSO, Lift Off, Project Astro, etc.

Page 14: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Variation in absorption of various elementsIndicative of varying density of the diskPossible Ring Structure

Page 15: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Eqw minimumEqw maximumLeadbeater/Stencel plateaus

Page 16: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Measure the days of a min or max

Find fraction of orbit this represents:width of ring = min or max days/(27.1 * 365)

Represent fraction angle (* 360)

Knowing the radius 18.1 AU, use small angle approximation (sin or tan) to find ring width

18.1 AU

Fraction of orbit= (20 days ) *360 (27.1*365)= 0.73

Ring Width = tan 0.73 * 18.1= 0.23 AU

Page 17: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Ring mins and maxs are roughly 0.2 AU

Page 18: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

1990 – S. Ferluga: disk is actually a series of concentric rings with gaps between them (like rings of Saturn)

Ferluga (1990, A&A, 238, 270)

Our result predict an outer ring at a radius of 3.3AU, a wider ring with radius 2.8 AU, and two

small inner rings with a radius near 1.5 AU. These

two small rings may represent the one inner ring. Our results are similar to Ferluga’s

prediction.

Our result predict an outer ring at a radius of 3.3AU, a wider ring with radius 2.8 AU, and two

small inner rings with a radius near 1.5 AU. These

two small rings may represent the one inner ring. Our results are similar to Ferluga’s

prediction.

Page 19: Sally Seebode Science Educator SMUHSD. Dean Drumheller, Steve Howell, Don Hoard, Sally Seebode, Darryl Stanford

Take data 2 or more times every week

Examine the spectra for more information: H alpha emission and absorption components

Changing molecular bands (CN, CH) FWHM interpretation