The Magellan Venus Probe Frank Koconis. Contents Venus compared to Earth Earlier exploration of...

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The Magellan Venus Probe Frank Koconis

Transcript of The Magellan Venus Probe Frank Koconis. Contents Venus compared to Earth Earlier exploration of...

Page 1: The Magellan Venus Probe Frank Koconis. Contents Venus compared to Earth Earlier exploration of Venus The problem: How to map the surface The Magellan.

The Magellan Venus Probe

Frank Koconis

Page 2: The Magellan Venus Probe Frank Koconis. Contents Venus compared to Earth Earlier exploration of Venus The problem: How to map the surface The Magellan.

Contents

• Venus compared to Earth• Earlier exploration of Venus• The problem: How to map the surface• The Magellan Mission• Working at JPL

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Venus Compared to Earth

Earth Venus

Diameter 12,742 km 12,104 km

Distance from Sun 150,000,000 km 108,000,000 km

“Day” (rotation period) 1 day 243 days

Year 365 days 228 days

Surface gravity 1 G 0.9 G

Atmospheric composition N2 (77%), O2 (21%), Ar (1%), C02 (0.4%)

C02 (96%), N2 (3%), traces of other gasses

Atmospheric pressure 1.0 92

Average surface temperature 15° C (59° F) 477° C (891° F)

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Earlier Exploration of Venus

From Earth, all we see is the clouds ->

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Earlier Exploration of Venus (cont.)So we have sent many unmanned probes thereName Year Sent By Notes

Mariner 2 1962 USA Fly-by at 34,745 km

Venera 4 1967 Russia (USSR) Entered atmosphere

Mariner 5 1967 USA Fly-by at 4023 km

Venera 5 1969 Russia (USSR) Descended into atmosphere by parachute

Venera 6 1969 Russia (USSR) Descended into atmosphere by parachute

Venera 7 1970 Russia (USSR) Soft-landed on surface; survived 23 min.

Venera 8 1972 Russia (USSR) Soft-landed on surface

Mariner 10 1973 USA Fly-by en-route to Mercury

Venera 9 1975 Russia (USSR) Soft-landed and transmitted pictures

Venera 10 1975 Russia (USSR) Landed; transmitted pictures for 65 min.

Pioneer 12 1978 USA Orbited and mapped surface using radar

Pioneer 13 1978 USA Entered atmosphere

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Earlier Exploration of Venus (cont.)…more than to any other planetName Year Sent By Notes

Venera 11 1978 Russia (USSR) Soft-landed

Venera 12 1978 Russia (USSR) Soft-landed but failed to return images

Venera 13 1981 Russia (USSR) Soft-landed and sent color images

Venera 14 1981 Russia (USSR) Drilled into soil and took seismic readings

Venera 15 1983 Russia (USSR) Orbiter; mapped surface using radar

Venera 16 1983 Russia (USSR) Orbiter; mapped surface using radar

Vega 1 1984 Russia (USSR) Dropped balloon probe en-route to Halley’s

Vega 2 1984 Russia (USSR) Dropped balloon probe en-route to Halley’s

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The Surface of Venus (Venera 9)

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The Problem: How to Map the Surface

• You can’t see through the clouds• BUT- Radar can go through• Using radar to map the topography of Venus– Earth-based radar: many attempts starting in the 1940’s– Pioneer 12: produced a map with about 100 km resolution– Venera 15 and 16: produced map with 2 km resolution– Magellan

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The Magellan Mission

• Named after Ferdinand Magellan– Led first round-the-globe voyage (1519 – 1522)– Killed in a dispute between tribes in the Philippines, but

one of his ships completed the trip

• Magellan mission to Venus– Developed by the Jet Propulsion Lab and Martin Marietta– Launched on May 4, 1989– Reached Venus on August 7, 1990– End of mission: October 13, 1994

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The Magellan Mission- The Probe

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The Magellan Mission- Launch

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The Magellan Mission- Getting There

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The Magellan Mission- Mapping Venus

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The Magellan Mission- Polar Orbit

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The Magellan Mission- Results

• Goal was to map 70% of surface, to 100m resolution• Actually mapped 98%!

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The Magellan Mission- Results

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The Magellan Mission- Aphrodite Terra

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The Magellan Mission- Maat Mons

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The Magellan Mission- Addams Crater

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The Magellan Mission- My Role

• On-board computer was called CDS (Command and Data Subsystem)– Much less powerful than a smartphone– Operated the probe with no assistance from Earth– New instructions sent once per week

• My role: testing the CDS (1984 – 1985)– CDS needed to detect and handle failures in spacecraft

components– To test this, a rack of test computers was built, each acting

as one component of the probe– Our team programmed these test computers

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Working at JPL

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JPL: The Campus

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JPL: Spacecraft Assembly Facility

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JPL: Deep-Space Network

Three sites: California, Australian and Spain

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JPL: Tracking Facility

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JPL: Museum

Ranger 7

Pioneer 1 Explorer 1

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Frank Koconis• Education– Myers Park High School: Class of 1980– Georgia Institute of Technology: Class of 1984

• Bachelor of Science in Computer Science, with High Honors

– University of NC at Charlotte: 1992• Master of Science in Computer Science• Attended evening classes while working full time

• After JPL…– JPL was my first job after Georgia Tech– Since then, I have worked in many different industries

including telecommunications, textiles, government, teaching, petroleum and banking

– Currently working for Syncsort

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Questions?

Web Linkshttp://en.wikipedia.org/wiki/Magellan_%28spacecraft%29http://www2.jpl.nasa.gov/magellan/guide.htmlhttp://nssdc.gsfc.nasa.gov/planetary/factsheet/venusfact.htmlhttp://www.astronomynotes.com/tables/tablesb.htmhttp://sci.esa.int/science-e/www/object/index.cfm?fobjectid=34067http://nssdc.gsfc.nasa.gov/nmc/spacecraftDisplay.do?id=1989-033Bhttp://yooperabroad.wordpress.com/2012/07/31/nasa-jet-propulsion-lab/