Prospect for UV observations from the Moon
arXiv:1410.3266 · doi:10.1007/s10509-014-2056-y
Abstract
Space astronomy in the last 40 years has largely been done from spacecraft in low Earth orbit (LEO) for which the technology is proven and delivery mechanisms are readily available. However, new opportunities are arising with the surge in commercial aerospace missions. We describe here one such possibility: deploying a small instrument on the Moon. This can be accomplished by flying onboard the Indian entry to the Google Lunar X PRIZE competition, Team Indus mission, which is expected to deliver a nearly 30 kgs of payloads to the Moon, with a rover as its primary payload. We propose to mount a wide-field far-UV (130--180 nm) imaging telescope as a payload on the Team Indus lander. Our baseline operation is a fixed zenith pointing but with the option of a mechanism to allow observations of different attitudes. Pointing towards intermediate ecliptic latitude (50 deg or above) ensures that the Sun is at least 40 deg off the line of sight at all times. In this position, the telescope can cover higher galactic latitudes as well as parts of Galactic plane. The scientific objectives of such a prospective are delineated and discussed.
28 pages, 8 figures
References in corpus (31)
- One or more bound planets per Milky Way star from microlensing observations
- An ultraviolet-optical flare from the tidal disruption of a helium-rich stellar core
- Stellar Processes Near the Massive Black Hole in the Galactic Center
- Luminous Thermal Flares from Quiescent Supermassive Black Holes
- The early UV/Optical emission from core-collapse supernovae
- Ultraviolet tails and trails in cluster galaxies: A sample of candidate gaseous stripping events in Coma
- Discovery of a Ringlike Dark Matter Structure in the Core of the Galaxy Cluster Cl 0024+17
- Supernova Shock Breakout from a Red Supergiant
- GALEX Ultraviolet Imaging of Dwarf Galaxies and Star Formation
- Caught in the Act: Strong, Active Ram Pressure Stripping in Virgo Cluster Spiral NGC 4330
- Probing Shock Breakout with Serendipitous GALEX Detections of Two SNLS Type II-P Supernovae
- Collisional Excavation of Asteroid (596) Scheila
- The Extraordinary Multi-Tailed Main-Belt Comet P/2013 P5
- Sgr A* flares: tidal disruption of asteroids and planets?
- The GALEX Time Domain Survey I. Selection and Classification of Over a Thousand UV Variable Sources
- SN 2009kf : a UV bright type IIP supernova discovered with Pan-STARRS 1 and GALEX
- Tidal disruption of a super-Jupiter by a massive black hole
- The nature of the DLS fast transients
- The 1 um discontinuity in the Extragalactic Background Light spectrum: an artefact of foreground subtraction
- A cryogenic liquid-mirror telescope on the moon to study the early universe
- Planets in the Early Universe
- A Simple Explanation for DAMA with Moderate Channeling
- The Diffuse Ultraviolet Foreground
- On the Binary Nature of Dust-encircled BD+20 307
- Mass and motion of globulettes in the Rosette Nebula
- Far Ultraviolet Emission in the A2597 and A2204 Brightest Cluster Galaxies
- The Chelyabinsk superbolide: a fragment of asteroid 2011 EO40?
- GALEX FUV Observations of Comet C/2004 Q2 (Machholz): The Ionization Lifetime of Carbon
- Ultraviolet Spectroscopy of Asteroid (4) Vesta
- Prospects for Observations of Transient UV Events with the TAUVEX UV Observatory
- Large Scale Extinction Maps with UVIT
Cited by in corpus (3)
- Prospect for UV observations from the Moon. II. Instrumental Design of an Ultraviolet Imager LUCI
- Prospect for UV observations from the Moon. III. Assembly and ground calibration of Lunar Ultraviolet Cosmic Imager (LUCI)
- The Near Ultraviolet Transient Surveyor (NUTS): An ultraviolet telescope to observe variable sources