Introduction Observing Statistics Curriculum Research Technology Sample Images Links

Rigel Acceptance Tests

Results of the June 2002 acceptance tests are now available.

Design Criteria

The Rigel robotic observatory system design was driven by six criteria:

  1. The telescope, camera, and spectrometer must be capable of producing high quality images and spectra well suited to a wide variety of undergraduate astronomy laboratory education and research projects

  2. The Observatory control software must be intelligent, robust, and intuitive. It must be easy to operate by non-technically trained users, with comprehensive safety features to prevent damage by inappropriate user input.

  3. The Observatory enclosure must be capable of fail-safe, weather-tight closure in the event of power outage or severe weather

  4. The Observatory and its enclosure must be easily sited on a variety of settings, with a minimum of site requirements: typically a small concrete pad, electricity, and Internet connectivity.

  5. The Observatory control, image and spectral analysis, and curriculum software suite must be tightly integrated, extensible, and Web-based as much as possible to allow maximum

  6. The design must achieve the design goals at the lowest possible total cost.

After considerable discussion of these design criteria with the telescope design group at Torus Precision Optics and the chief software engineer at Clear Sky Institute, as well as extensive experience with existing automated telescopes at the University of Iowa, we have designed a system that meets the above criteria. The complete system, called Rigel, can be produced in quantity at reasonable cost and with proven components and materials

Description

The Rigel robotic observatory consists of a 37 cm (14.5in) diameter f/14 Cassegrain reflector, equatorial mount, filter wheel, high QE cooled CCD imaging camera, CCD-based spectrometer, and fiberglass dome enclosure. All components are fully controlled by a single computer which can be operated using standard Ethernet and Internet protocols. This allows the Observatory to be located anywhere the user finds convenient, from the roof top of a local campus building to any remote site with adequate power and Internet connections.

A table of specifications for the Rigel system is given in the table below, followed by a table of performance specifications. Based on previous experience with the Automated Telescope Facility and the Iowa Robotic Telecope, these specifications are well matched to most observing projects in undergraduate astronomy laboratories.

 

 

Rigel Hardware Specifications

SubSystem

Vendor, Model

Item

Specification

Optics

Torus Precision Optics modified CC-04 design

Optical Tube Assembly

Open Truss

Primary Mirror

37 cm (14.5in) diameter

1/16 wave RMS

Overall Focal Ratio

f/14

Optical Design

Classical Cassegrain

Mount design

Fork-mount Equatorial

Mount

Torus Precision Optics modified CC-04

Motors and Electronics

Steppers, CSI motion control

CCD Camera

FLI with SITe-003 sensor

Camera assembly

1024x1024 24m sensor TE cooled, back-side illuminated, AR coated

Filter Wheel

Torus Precision Optics

Wheel assembly

Twelve position, stepper motor

Filters

Johnson-Cousins CBVRI, narrow band optional

Control Software

Torus

Talon observatory control software

Fully automated control of focus, mount, camera, filter wheel, dome, weather monitor, communication

Enclosure

Winer Observatory

Roll-off roof

Controlled by Talon software

Weather System

Davis Instruments

Weather Monitoring Equipment

Full local weather monitoring

Time Standard

-

NTP

<1 msec synchronization with UTC

Control Computer

Dell

Pentium 4 1.8 GHz, 512 MB RAM, 40 GB disk

Linux O/S

Server Compurter

Dell

PIII 700 MHz 2 x 27 GB disks 256 MB RAM

Linux O/S

Rigel Performance Specifications

Subsystem

Specification

Value

Mount

Pointing error

30 arcsec RMS full sky

Tracking error

<0.01 arcsec per second

Optics

Surface Error

<0.2l wave peak to valley

<0.06l RMS

Point Spread Function

>88% of stellar photons within one pixel (24m) at sensor edge (6.1mm)

Imaging

Field of View

17.1 arcmin

Pixel Resolution

0.98 arcsec

Sensitivity

>10:1 SNR 19th magnitude star with clear filter  in 60 seconds

Spectroscopy

Spectral Resolution

1.5 nm

Total Spectrum Coverage

400 – 750 nm continuous

Sensitivity

>100:1 SNR on 6th magnitude  star in 10 sec.

Design Drawings

Item
Date
Comment
Mount base: Front view, Side view 6 Oct 2000 Series II design, same as CC04-CC05
Isometric of complete telescope, Front view, Side view 6 Oct 2000  

 

Contact: rigel@phobos.physics.uiowa.edu

Last updated December 2, 2003