recent studies of mars: 2013-2014

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Recent Studies of Mars: 2013-2014 Richard W. Schmude, Jr. Gordon State College Barnesville, GA

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Recent Studies of Mars: 2013-2014. Richard W. Schmude, Jr. Gordon State College Barnesville, GA. Overview. Purpose of work North Polar Cap (NPC) Hellas Brightness measurements. Purpose. NPC interannual variability Hellas variability Time of day Year season - PowerPoint PPT Presentation

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Page 1: Recent Studies of Mars: 2013-2014

Recent Studies of Mars: 2013-2014

Richard W. Schmude, Jr. Gordon State College

Barnesville, GA

Page 2: Recent Studies of Mars: 2013-2014

Overview

• Purpose of work

• North Polar Cap (NPC) • Hellas

• Brightness measurements

Page 3: Recent Studies of Mars: 2013-2014

Purpose

• NPC interannual variability

• Hellas variability– Time of day– Year– season

• Brightness (visible & Near infrared)

Page 4: Recent Studies of Mars: 2013-2014

Hubble Image Processed by P. James, T. Clancy, S. Lee and NASA

Page 5: Recent Studies of Mars: 2013-2014

Introduction: Ls

Ls range Season (N. hemisphere)0 – 90° Spring

90 – 180° Summer180 – 270° Fall

270 – 0° Winter

Page 6: Recent Studies of Mars: 2013-2014

Voting Questions

• Do not talk to anyone until after 1st vote

• After 1st vote– Talk to someone that you disagree with– Convince him/her that you are right– Listen to your partner

Page 7: Recent Studies of Mars: 2013-2014

Voting Question

• If Ls = 135° it is ___________ in the northern hemisphere.

a. late spring b. mid springc. early summer d. mid summer

Page 8: Recent Studies of Mars: 2013-2014

Voting Question

Ls = 50° is similar to _______ in the USA.

a. February b. Junec. October d. May

Page 9: Recent Studies of Mars: 2013-2014

Method and Materials

• WinJupos– Name an image• 2014-07-12-1320-name & other info.

– Load an image– Software computes longitude & latitude

Page 10: Recent Studies of Mars: 2013-2014

Polar Cap MeasurementGoal: get all longitudes

Page 11: Recent Studies of Mars: 2013-2014

NPC: Mean latitude

Page 12: Recent Studies of Mars: 2013-2014

Hellas measurements

• Northern border measured– Every 5° of longitude– 270° W to 320° W– Red light images used– Mean values computed for each 5° of longitude

Page 13: Recent Studies of Mars: 2013-2014

Why red light?green-left & red-right

Page 14: Recent Studies of Mars: 2013-2014

Results: NPC in 2013 – 2014

Page 15: Recent Studies of Mars: 2013-2014

Interannual variability

• Spring NPC – Mean latitudes (all longitudes) considered– Wilcoxon Signed Rank Test• 90% confidence level• As few as five values • Non-parametric test

Page 16: Recent Studies of Mars: 2013-2014

Data sets

• MGS: 2000, 2002, 2006*, 2007-08*

• Schmude: 2009-10, 2011-12, 2013-14

• Individual latitudes are not reported

Page 17: Recent Studies of Mars: 2013-2014

ResultsYear D mean latitude Comparison to 20002000 --- The standard2002 0.9° Larger2006 ~0.2° Probably the same

2007-08 ~0.6° Probably smaller2009-10 0.8° Larger2011-12 0.3° Same2013-14 0.0° Same

Page 18: Recent Studies of Mars: 2013-2014

Voting Question

At Ls = 50°, the temperatures are __________ in the southern hemisphere of Mars.

a. rising b. falling

Page 19: Recent Studies of Mars: 2013-2014

Hellas: white layer

• Northern border– Clouds or frost?– Growth during fall?– Changes from morning to afternoon?– Interannual differences?

Page 20: Recent Studies of Mars: 2013-2014

Hellas: white layer

Page 21: Recent Studies of Mars: 2013-2014

Hellas: changes in Northern border

• Wilcoxon Signed Rank Test– Mid fall (1995) and late fall – early winter (2014)– Morning afternoon (2014)– 2012 and 2014 (similar seasons)

Page 22: Recent Studies of Mars: 2013-2014

Statistical results: Hellas

• There is no statistical difference (90% conf.)– Mid fall and late fall/early winter– Morning and afternoon– 2012 and 2014 (similar seasons)

Page 23: Recent Studies of Mars: 2013-2014

Brightness Measurements

• Purpose– Long-term changes– Water reservoirs– Dust storms– Brightness model of planet

Page 24: Recent Studies of Mars: 2013-2014

Brightness in Magnitudes

• Zero magnitude = a flux of light

• As magnitude drops, brightness increases

Page 25: Recent Studies of Mars: 2013-2014

Electromagnetic Radiation

• Electric wave • Magnetic wave• Velocity = 186,000 miles/hour (vacuum)• Wavelength (length of one wave)

Page 26: Recent Studies of Mars: 2013-2014

Electromagnetic radiationWavelength and color

Filter Wavelength ColorV 540 nm greenR 700 nm redJ 1250 nm noneH 1650 nm none

Page 27: Recent Studies of Mars: 2013-2014

Previous work

• Schmude measured B, V, R and I brightness of Mars from 1991 to 2014

• Mallama (2007) summarizes work up to 2005.

• Almost no work done for J and H filters

Page 28: Recent Studies of Mars: 2013-2014

Near Infrared light

Page 29: Recent Studies of Mars: 2013-2014

Voting question

Please rank the objects from highest to lowest magnitude.

a. Sun, full Moon, Venusb. Sun, Venus, full Moonc. Full Moon, Venus, Sund. Venus, full Moon, Sun

Page 30: Recent Studies of Mars: 2013-2014

Materials

• SSP-4 photometer• Celestron CG-4 mount• 0.09 m Maksutov telescope• Extension cord (requires AC power)

Page 31: Recent Studies of Mars: 2013-2014

Experimental set-up

Page 32: Recent Studies of Mars: 2013-2014

Method of brightness measurement

• Sky brightness and then comparison star• Sky brightness and then Mars• Repeat 2 ½ more times

• Compute Mars’ magnitude• Make corrections

Page 33: Recent Studies of Mars: 2013-2014

Normalized Magnitude J(1,0) and H(1,0)

• Mars is 1 au from Earth and Sun

• Sunlight reflects directly back to observer (zero phase angle)

Page 34: Recent Studies of Mars: 2013-2014

Results: Albedo

Page 35: Recent Studies of Mars: 2013-2014

Light curve J filter

Page 36: Recent Studies of Mars: 2013-2014

Light curve H filter

Page 37: Recent Studies of Mars: 2013-2014

Conclusions

• NPC may undergo small changes from one year to the next

• Hellas white area: No change with respect to diurnal, seasonal or year to year cycles

• Mars’ albedo does not rise in near infrared

• Mars brightens as it rotates in the J & H filters