Supplement to photographic catalog of selected planetary size comparisons

Bibcode
1991stpc.book.....M
Meszaros, Stephen Paul
Bibliographical reference

Supplement to photographic catalog of selected planetary size comparisons NASA

Advertised on:
6
1991
Number of authors
1
IAC number of authors
0
Citations
0
Refereed citations
0
Description
This document updates and extends the photographic catalog of selected planetary size comparisons. It utilizes photographs taken by NASA spacecraft to illustrate size comparisons of planets and moons of the solar system. Global views are depicted at the same scale, within each comparison, allowing size relationships to be studied visually.
Type
Non-refereed
Solar system

It may interest you

  • Non-refereed
    Performance of the image persistence model for Euclid infrared detectors
    Large-format infrared detectors are at the heart of major ground and space-based astronomical instruments, and the HgCdTe HxRG is the most widely used. The Near Infrared Spectrometer and Photometer (NISP) of the ESA's Euclid mission launched in July 2023 hosts 16 H2RG detectors in the focal plane. Their performance relies heavily on the effect of
    Kubik, B. et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13103E..15K
    Citations
    0
  • Non-refereed
    HARMONI at ELT: athermal toroidal mirror mount for HARMONI pre-optics
    HARMONI is the high angular resolution optical and near-IR integral field spectrograph for the Extremely Large telescope (ELT). It covers a large spectral range from 470nm to 2450nm with resolving powers from 3300 to 18000 and spatial sampling from 60mas to 4mas. The Instrument Pre-Optics (IPO), a sub-system under the responsibility of the
    Hernández, Elvio et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13100E..34H
    Citations
    0
  • Non-refereed
    HARMONI at ELT: project status and instrument overview
    HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 450 nm to 2450 nm with resolving powers from 3500 to 18000 and spatial sampling from 60 mas to 4 mas. It can operate in two Adaptive Optics modes - SCAO (including a High Contrast capability) and LTAO - or with NOAO. The
    Thatte, Niranjan A. et al.

    Advertised on:

    7
    2024
    Bibcode
    2024SPIE13096E..14T
    Citations
    0