Abstract
The James Webb Space Telescope (JWST) has the potential to enhance our understanding of near-Earth objects (NEOs). We present results of investigations into the observability of NEOs given the nominal observing requirements of JWST on elongation (85°–135°) and non-sidereal rates (<30 mas s−1). We find that approximately 75% of NEOs can be observed in a given year. However, observers will need to wait for appropriate observing windows. We find that JWST can easily execute photometric observations of meter-sized NEOs that will enhance our understanding of the small NEO population.
Original language | English (US) |
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Pages (from-to) | 1-6 |
Number of pages | 6 |
Journal | Publications of the Astronomical Society of the Pacific |
Volume | 128 |
Issue number | 959 |
DOIs | |
State | Published - Jan 2016 |
Externally published | Yes |
Keywords
- Asteroids: general
- Minor planets
- Telescopes
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science