ISO 14490-4:2005
Optics and optical instruments — Test methods for telescopic systems — Part 4: Test methods for astronomical telescopes
Optics and optical instruments — Test methods for telescopic systems — Part 4: Test methods for astronomical telescopes
- Статус документа:
- Действующий
- Формат:
- Электронный (PDF)
- Количество страниц:
- 8
- Дата публикации:
- 4 ноября 2005 г.
- Издание:
- ISO IS 14490 edition 1 version 1
- ICS:
- 37.020
ISO 14490-4:2005 is applicable to amateur astronomical telescopes. For general optical test methods of telescopic systems see ISO 14490-1.
Abstract
Overview
ISO 14490-4:2005 - Optics and optical instruments: Test methods for astronomical telescopes specifies standardized optical test methods applicable to amateur astronomical telescopes. It is Part 4 of the ISO 14490 series and focuses on practical, repeatable measurements of key telescope characteristics such as clear aperture, focal length and resolution. For general telescopic system test methods, refer to ISO 14490-1.
Key topics and technical requirements
- Scope: Applies to amateur astronomical telescopes; uses terminology from ISO 14132-1 and ISO 14132-4.
- Clear aperture measurement: Three accepted procedures:
- Direct linear measurement of objective lens or primary mirror.
- Collimator method: project a bundle of parallel rays and measure the exit pupil diameter on a screen.
- Diffuse‑illumination/travelling microscope method using ground glass and measuring in object space.
- Focal length measurement:
- Nodal slide (rotary table) method for refracting objectives and eyepieces - align nodal plane to axis of rotation and determine focal length from microscope position differences.
- Mirror method for reflecting objectives - use a microscope with illuminator and measure positions for direct and reflected reticle images; focal length equals half the difference in readings (not applicable to centrally obscured mirrors).
- Resolution testing:
- Main telescope resolution is measured with a collimator and a two‑pinhole test target sized per the Rayleigh criterion (ISO 14132-4), observed through a high-quality eyepiece and by an observer with visual acuity per ISO 8596.
- Recommended collimator focal length > 2000 mm; example pinhole separations are provided for common angular separations.
- Reporting requirements: Test reports must include method, date, specimen ID, test arrangement details (if deviating), reference to ISO 14490-4:2005, laboratory and examiner names.
Applications and who uses it
- Manufacturers of consumer and amateur astronomical telescopes for quality control and product specifications.
- Metrology and test laboratories performing acceptance testing, verification, or certification.
- Optical engineers and designers validating objective and eyepiece performance.
- Retailers and consumer organizations assessing product claims (e.g., aperture, focal length, resolving power).
- Hobbyist advanced users and clubs can use the standard to understand test protocols and interpret manufacturer data.
Related standards
- ISO 14490-1: Test methods for basic characteristics (general methods for telescopic systems)
- ISO 14490 series (Parts 2–7 cover binoculars, sights, transmittance, veiling glare, limit of resolution)
- ISO 14132-1 and ISO 14132-4: Vocabulary and terms for telescopic systems
- ISO 8596: Visual acuity testing (used in resolution measurement)
Keywords: ISO 14490-4:2005, astronomical telescopes, test methods, focal length measurement, clear aperture, resolution test, amateur astronomical telescopes, collimator, nodal slide.
Технические детали
- Технический комитет
- ISO/TC 172/SC 4 - Telescopic systems
- SKU
- ISO 14490-4:2005
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