Hungaria asteroid region telescopic spectral survey (HARTSS) I: Stony asteroids abundant in the Hungaria background population

Earth and Planetary Sciences

• Ordinary Chondrite 100%
• Achondrite 100%
• Mineralogy 75%
• Chondrite 75%
• Chladnite 75%
• Acapulcoite 75%
• Infrared Spectra 50%
• Spectral Band 50%
• Terrestrial Planet 50%
• Parent Body 50%
• Olivine 25%
• Reflectance 25%
• Infrared Telescopes 25%
• Orthopyroxene 25%
• Asteroid Belts 25%

Keyphrases

• Asteroids 100%
• Spectral Survey 100%
• Background Population 100%
• Hungarias 100%
• Band Parameters 25%
• Ordinary Chondrites 20%
• σ-complexes 20%
• Primitive Achondrites 20%
• Acapulcoite 15%
• Mineralogy 10%
• Surface Composition 10%
• Source Area 10%
• Telescope Facilities 10%
• Near-infrared Spectrum 10%
• Icarus 10%
• Spectral Bands 10%
• Compositional Diversity 10%
• Terrestrial Planets 10%
• Parent Body 10%
• Chondrite Meteorites 10%
• Aubrites 10%
• H Chondrite 10%
• Laboratory Research 5%
• Space Telescope 5%
• Infrared Telescopes 5%
• Inner Boundary 5%
• Olivine 5%
• Family Members 5%
• Survivors 5%
• Surface Mineralization 5%
• Parameter Analysis 5%
• Asteroid Belt 5%
• Preserved Samples 5%
• Orthopyroxene 5%
• Non-family 5%
• Main Belt 5%
• Background Objects 5%
• C-complex 5%
• Enstatite Achondrites 5%
• Telescopio Nazionale Galileo 5%
• Near Infrared Reflectance Spectra 5%
• Clan 5%
• L Chondrite 5%
• Diagnostic Absorption Feature 5%
• Current Resonance 5%
• Spectral Diversity 5%
• Near-infrared Instruments 5%
• Giant Planet Migration 5%
• Complex Background 5%
• Parameter Measurement 5%
• Purgatory 5%
• Resonance Structures 5%
• Surface Potential 5%
• Body Remains 5%