near-shoemaker mission to 433 eros

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Cospar Capacity Building Workshop On Planetary Science N e a r E a r t h A s t e r o i d R e n d e z v o u s Dr. Lucy McFadden July 30, 2007 NEAR-Shoemaker Mission to 433 Eros

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NEAR-Shoemaker Mission to 433 Eros. N e a r E a r t h A s t e r o i d R e n d e z v o u s. Cospar Capacity Building Workshop On Planetary Science. Dr. Lucy McFadden July 30, 2007. Scientific Objectives. - PowerPoint PPT Presentation

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Page 1: NEAR-Shoemaker Mission to 433 Eros

Cospar Capacity Building WorkshopOn

Planetary Science

N e a r E a r t h A s t e r o i d R e n d e z v o u s

Dr. Lucy McFadden

July 30, 2007

NEAR-Shoemaker Missionto 433 Eros

NEAR-Shoemaker Missionto 433 Eros

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Scientific ObjectivesScientific Objectives

• Determine physical and chemical properties of 433 Eros

• Address major questions: – formation of the Solar

System

Page 4: NEAR-Shoemaker Mission to 433 Eros

Eros’ Orbital PropertiesEros’ Orbital Properties

• Mars-crossing• i=10.8°• Orbital period= 1.76 y• Rotation period=5.27hr

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Journey to ErosBei dem WaldgottJourney to Eros

Bei dem Waldgott

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Launched Feb. 17, 1996Launched Feb. 17, 1996

• Delta 7925 launch vehicle

• Cape Canaveral

QuickTime™ and aVideo decompressor

are needed to see this picture.

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SpacecraftSpacecraft

• Fixed solar panels• 1.5 m high-gain

antenna• 6 instruments

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QuickTime™ and aVideo decompressor

are needed to see this picture.

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253 Mathilde253 Mathilde

• June 27,1997• 1212 km flyby • C-type asteroid• 66 x 48 x 44 km• Albedo = 0.047• =1.340± 200 kg/m3

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Earth SwingbyEarth Swingby

• Jan. 23, 1998• 106.300 - 306.600 km• Trajectory maneuver

– Match inclination

– i=10

• Test and calibrate instruments

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Psyche in der untweltPsyche in der untwelt

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Engine burn abort/Eros flyby

Engine burn abort/Eros flyby

• December 20, 1998– Aborted maneuver

– +27 hrs regained contact

• December 23, 1998– 3827 km flyby

• January 3, 1999– Bipropellant burn

– Feb. 2000 rendezvous

Page 14: NEAR-Shoemaker Mission to 433 Eros

Psyche for VenusPsyche for Venus

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Fundamental PropertiesFundamental Properties

• Mass=6.687 ± 1015 kg• Volume=2550 km3

• kg/m3

• Size=32x8x8 km• Rotation pole

– RA 11.4°– Dec 17.3°±0.1

Page 16: NEAR-Shoemaker Mission to 433 Eros

Eros : Major QuestionsEros : Major Questions

• Is Eros a fragment or agglomerate?

• Is Eros’ composition primitive or differentiated?

• Does it have a magnetic field?

• Are there satellites?

Page 17: NEAR-Shoemaker Mission to 433 Eros

ShapeShape

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Near-IR SpectroscopyNear-IR Spectroscopy

• Low phase flyby 0-50°• >5600 spectra • 800-2500 nm• 12 -2.5 km/spectrum

– 0.76 x 0.38° slit

• 1st spatially resolved spectra

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Mineral Structure

The pyroxene group is composed of minerals of the general formula XYSi2O6, where X and Y are two divalent cations and occupy twoStructurally different sites. If X and Y are the same small-radius divalent cation like Fe or Mg the resultant structure is commonly orthorhombic, giving us the orthopyroxene group.

Orthopyroxene

Olivine

The olivine group is composed of minerals of the general formula X2SiO4 where X = Mg ,Fe2+, or Ca; Y = Al, Cr, or Fe3+; and Z = Si. The X-site is 8 coordinated, the Y -site is 6-coordinated (octahedral) and the Z-site is 4-coordianted

Clinopyroxene

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Page 21: NEAR-Shoemaker Mission to 433 Eros

Low Phase Flybyfor SpectroscopyLow Phase Flybyfor Spectroscopy

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Page 23: NEAR-Shoemaker Mission to 433 Eros

Spatially Resolved Spectroscopy

Spatially Resolved Spectroscopy

• Variations in band depth and spectral slope– Range 1-4%

– Includes phase angle corrections

– Homogeneous to 4%

– At 3 km resolution

Page 24: NEAR-Shoemaker Mission to 433 Eros

Map of 1-µm Band DepthMap of 1-µm Band Depth

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Laser Rangefinder-lidarLaser Rangefinder-lidar

• Nd:YAG laser rangefinder

• First detections from Eros at 290 km

• Measures distance to surface along line of sight

Page 29: NEAR-Shoemaker Mission to 433 Eros

MagnetometerMagnetometer

• Three-axis fluxgate magnetometer

• No magnetic field detected

• Sensitivity of 1 nT

• Upper limit at 200 km orbit is B=30,000 nt (earth-like)

Page 30: NEAR-Shoemaker Mission to 433 Eros

Global Rotation 2 Days after

going into orbit around Eros

Global Rotation 2 Days after

going into orbit around Eros

Page 31: NEAR-Shoemaker Mission to 433 Eros

200 km orbit200 km orbit

Page 32: NEAR-Shoemaker Mission to 433 Eros

100 Km orbit100 Km orbit

Page 33: NEAR-Shoemaker Mission to 433 Eros

Psyche CraterPsyche Crater

Page 34: NEAR-Shoemaker Mission to 433 Eros

Psyche is the same size as Barringer Crater Arizona,

US

Psyche is the same size as Barringer Crater Arizona,

US

Page 35: NEAR-Shoemaker Mission to 433 Eros

Low Altitude Flyover Oct. 26

Low Altitude Flyover Oct. 26

Page 36: NEAR-Shoemaker Mission to 433 Eros

X-ray Gamma-Ray Spectrometer

X-ray Gamma-Ray Spectrometer

• First detections – class X solar flare

• Mg, Fe, Ca– Verified calibrations

• Interplanetary Gamma Ray Burst Network– Earth orbiting satellites

and Ulysses s/c– Location of optical and

radio counterparts

Page 37: NEAR-Shoemaker Mission to 433 Eros

X-ray and -ray spectroscopy

• Data acquired during 5 solar flares and during two extended “quiet Sun” periods.

• Large systematic uncertainties, but relative ratios are reliable.

• Primitive, undifferentiated ratios of– Mg/Si, Al/Si, Ca/Si and Fe/Si

• global differentiation is ruled out.• S/Si is below chondritic values• Nittler et al. 2001 MAPS, 36, 1673-1695

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End of MissionEnd of Mission

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http://near.jhuapl.eduhttp://near.jhuapl.edu

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Science Team LeadersScience Team Leaders

• Tom Coughlin• Andy Cheng• Joe Veverka

• Jacob Trombka• Bill Boynton• Mario Acuna• Maria Zuber

Page 45: NEAR-Shoemaker Mission to 433 Eros

Science Team MembersScience Team Members

• J.P. Barriot• James F. Bell• Mark Robinson• Scott Murchie• Michael Malin• Clark Chapman• Lucy McFadden

• William Boynton• Christopher Russell• Alexander Konopliv• Steven Squyres• Peter C. Thomas• Johannes Brueckner