pluto occultation
DESCRIPTION
Pluto Occultation. 20/21 August 2002. Occultation Sequence. 7:31 UT. 5:33 UT. 6:26 UT. 7:03 UT. Pluto. Charon. P131 .1. Occultations by Pluto. 2002 P131.1. Pluto + Star. Pluto only. Williams’s light curve from August 2002, taken at University of Hawaii 2.2-m telescope. - PowerPoint PPT PresentationTRANSCRIPT
Pluto Occultation20/21 August 2002
Occultation Sequence
Pluto
CharonP131.1
5:33 UT 6:26 UT 7:03 UT 7:31 UT
Occultations by PlutoOccultations by Pluto
2002P131.1
Pluto + Star
Pluto only
Williams’s light curve from August 2002, taken at University of Hawaii 2.2-m telescope
Pasachoff, Jay M., Steven P. Souza, Bryce A. Babcock, David R. Ticehurst (Williams College); James L. Elliot, M. J. Person, and Kelly B. Clancy (MIT); Lewis C. Roberts, Jr., and Doyle T. Hall (Boeing Co., Maui); and David J. Tholen (U. Hawaii) 2005, "The Structure of Pluto's Atmosphere from the 2002 August 21 Stellar Occultation," Astron. J., 129, 1718-1723.
Occultation by PlutoOccultation by Pluto
2002P131.1
Pluto + Star
Pluto only
Williams’s light curve from August 2002, taken at University of Hawaii 2.2-m telescope
Pasachoff, Jay M., Steven P. Souza, Bryce A. Babcock, David R. Ticehurst (Williams College); James L. Elliot, M. J. Person, and Kelly B. Clancy (MIT); Lewis C. Roberts, Jr., and Doyle T. Hall (Boeing Co., Maui); and David J. Tholen (U. Hawaii) 2005, "The Structure of Pluto's Atmosphere from the 2002 August 21 Stellar Occultation," Astron. J., 129, 1718-1723.
Pluto + Star
Pluto only
Time (seconds after 8/21 06:40:00 UT)
Nor
mal
ized
Flu
x
0.8
1.0
0.6
0.4
0.0
0.2
450 500 600 650550 800700 750
UH 2.2-m/Williams CCD Light Curve
UH 2.2-m/Williams CCD Light Curve
0.75
0.8
0.85
0.9
0.95
1
1.05
300 400 500 600 700 800 900 1000
Nor
mal
ized
Flu
x
Time (seconds after 8/21 06:40:00 UT)
Half-light immersion time:2002 08 21: 06 47 59.3038 UT
Half-light emersion time:2002 08 21: 06 53 08.4001 UT
Duration: 5.15 minutes
Observations: Mauna Kea, 20 August 2002
Telescope: University of Hawaii 2.2 m f/10.14CCD: Princeton Instruments (Roper Scientific)
TE/CCD-576EFT frame-transfer CCDFrame Capture Rate = 2 Hz
Resolution: 0.2 arc sec pixelsunbinned for astrometric imagesbinned 5x5 for 20-min occultation run
Seeing: 0.4 arc sec
Support: Research Corporation
Technical Details
0.78
0.8
0.82
0.84
0.86
0.88
0.9
0.92
700 720 740 760 780 800
Nor
mal
ized
Flu
x
Time (seconds after 8/21 06:40:00 UT)
Zoom in of UH 2.2-m/Williams CCD Light Curve
Spikes, ingress and egress (flipped)
-0.2
0
0.2
0.4
0.6
0.8
1
1.2
100 110 120 130 140 150
UH_2.2BothWays.kg
Normalized Flux
Seconds after 2002 08 21 06 30 00
Haleakala data, I-bandAEOS Telescope/Boeing LTS
Comparison of Light Curves
Distance from Shadow Center (in units of half-light radius)
No
rma
lize
d S
tella
r F
lux
0.0
0.6
0.4
0.2
1.0
0.8
0.0–0.5–1.0 1.51.00.5–1.5
Changes in Pluto’s Atmospheric Pressure
Emersion (2002)Emersion
(1988)
2.0 6.0 8.04.0
1275
1255
1235
1215
Pressure (bar)
Rad
ius
(km
)
Papers published
"High-Time-Resolution White-Light Observations of Pluto's Occultation of P131.1 in
2002 August”
Elliot et al.
"The recent expansion of Pluto's atmosphere," Nature 424, 165-168, July 10, 2003.
Pasachoff et al.
Astronomical Journal paper on our data.
Person et al.
Meeting paper on the shape of Pluto’s atmosphere.