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Record W1618738724

A Deep-Field Infrared Observatory Near the Lunar Pole

2005· article· en· W1618738724 on OpenAlexvenueno aff
E. F. Borra, Omar Seddiki, J. R. P. Angel, S. P. Worden, D. Eisenstein, S. Silvanandam, Paul Hickson, M. A. Kastner

Bibliographic record

VenueJournal of the Royal Astronomical Society of Canada · 2005
Typearticle
Languageen
FieldPhysics and Astronomy
TopicPlanetary Science and Exploration
Canadian institutionsnot available
Fundersnot available
KeywordsTelescopePhysicsAstronomyObservatorySecondary mirrorField of viewOrbiterPrimary mirrorRemote sensingInfrared telescopeSkyInfrared astronomyInfraredOpticsGeology
DOInot available

Abstract

fetched live from OpenAlex

We have studied the feasibility and scientific potential of a 20 100 m aperture astronomical telescope at the lunar pole, with its primary mirror made of spinning liquid at less than 100K. Such a telescope, equipped with imaging and multiplexed spectroscopic instruments for a deep infrared survey, would be revolutionary in its power to study the distant universe, including the formation of the first stars and their assembly into galaxies. Our study explored the scientific opportunities, key technologies and optimum location of such a Lunar Liquid Mirror Telescope (LLMT). An optical design for a 20 m telescope with diffraction limited imaging over a 15-arcminute field has been developed. The LLMT could be used to follow up discoveries made with the 6 m James Webb Space Telescope, with more detailed images and spectroscopic studies, as well as to detect objects 100 times fainter, such as the first, high-red shift stars in the early universe. A model was made of a liquid mirror spinning on a superconducting bearing, as will be needed for the cryogenic, vacuum environment of the LLMT. Reflective silver coatings have been deposited for the first time on a liquid surface, needed to make infrared mirrors at ~ 80K. Issues relating to polar locations have been explored. Locations at or within a few km of a pole are preferred for deep sky cover, and allow for long integration times, by simple instrument rotation. In a collaborative effort with the European Space Agency’s SMART-1 lunar orbiter team, we obtained the first images of the North Pole in lunar winter. SMART-1 arrived at the Moon in November 2004 and has since spiraled down to a polar orbit. During the commissioning period and between orbit modifications, the orbiter imaged strips of Moon with its 5°× 5° AMIE camera. We analyzed available images of the North Pole region acquired during that period, which was close to the January 25th 2005 winter solstice. Our preliminary analysis shows ridges and crater rims within 0.5° of the North Pole are illuminated for at least some sun angles during lunar winter. Locations near these points may prove to be ideal for the LLMT. Lunar dust deposited on the optics or in a thin atmosphere, though unlikely, could be problematic. These issues should be further investigated in-situ and we propose a modest precursor site survey mission. RATIONALE FOR A LUNAR LIQUID MIRROR TELESCOPE (LLMT) Our lunar liquid mirror telescope concept is aimed at furthering our understanding of the early universe. This has recently been revolutionized by deep optical fields imaged first with the Hubble Space Telescope (HST), and followed up by observations by other telescopes across the electromagnetic spectrum, including

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.146
Threshold uncertainty score0.986

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.006
GPT teacher head0.179
Teacher spread0.172 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations3
Published2005
Admission routes1
Has abstractyes

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