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- 100 REM LIMITING MAGNITUDE OF A TELESCOPE
- 110 REM
- 120 INPUT "SCOPE APERTURE ";D : REM IN INCHES
- 130 INPUT "POWER ";MG : REM SCOPE'S MAGNIFICATION
- 140 INPUT "LIM MAG AT ZENITH ";MZ : REM FOR NAKED-EYE
- 150 INPUT "OBSERVER'S AGE ";AG : REM IN YEARS
- 160 INPUT "TELESCOPE TYPE (1-3) ";TT : REM 1=REFR, 2=REFL, 3=SCT
- 170 INPUT "CLEANLINESS (1-9) ";CL : REM 1=FILTHY, 9=CLEAN
- 180 INPUT "COLOR INDEX OF STAR ";CI : REM B-V MAGNITUDE
- 190 INPUT "ZENITH DISTANCE ";Z : REM IN DEGREES
- 200 INPUT "EXTINCTION COEFF ";KV : REM IN V-BAND
- 210 INPUT "SEEING DISK RADIUS ";SE : REM IN ARC-SECONDS
- 220 INPUT "EXPERIENCE (1-9) ";EX : REM 1=NOVICE, 9=VERY EXPER.
- 230 D=D*25.4 : REM CONVERT TO MM
- 240 IF TT=1 THEN DS=0 : REM NO OBSTRUCTION
- 250 IF TT=2 THEN DS=0.15*D : REM NEWT SECONDARY DIAM
- 260 IF TT=3 THEN DS=0.35*D : REM TYPICAL DIAM OF SCHMIDT-
- 270 REM CASS SECONDARY
- 280 Z=Z/57.296 : REM CONVERT TO RADIANS
- 290 CC=1.58E-10 : REM NIGHT-VISION CONSTANT
- 300 KK=0.0126 : REM NIGHT-VISION CONSTANT
- 310 K=1.2*KV : REM CORRECT KV TO 5100 A
- 320 X=1.0/COS(Z) : REM AIR MASS
- 330 IF TT=1 THEN FL=0.99^4 : REM 4 COATED SURFACES
- 340 IF TT=2 THEN FL=0.88^2 : REM 2 ALUMINIZED MIRRORS
- 350 IF TT=3 THEN FL=(0.99*0.88)^2 : REM CORRECTOR & 2 MIRRORS
- 360 FD=1.0-(DS/D)^2 : REM ALLOW FOR OBSTRUCTION
- 370 FO=0.99^4 : REM EYEPIECE (4 COATED
- 375 REM AIR-GLASS SURFACES)
- 380 DE=7*EXP(-0.5*(AG/100)^2) : REM DIAM EYE PUPIL IN MM
- 390 DP=D/MG : REM DIAM OF EXIT PUPIL
- 400 TH=2*SE*MG : REM APPARENT DIAMETER OF
- 410 REM SEEING DISK (ARC-SEC)
- 420 REM CORRECTIONS
- 430 FB=SQR(2) : REM BINOCULAR VISION
- 440 FE=10^(0.4*K*X) : REM ATMOSPHERIC EXTINCTION
- 450 FT=1/(FL*FD*FO-0.01*(9-CL)) : REM TOTAL TRANSMISSION
- 460 REM OF TELESCOPE
- 470 FPX=1.0 : REM LIGHT OUTSIDE PUPIL
- 480 IF DE<DP THEN FPX=(DP/DE)^2
- 490 FA=(DE/D)^2 : REM LIGHT-COLLECTING AREA
- 500 FM=MG^2 : REM SPREAD OF SKY PHOTONS
- 510 FR=1.0 : REM POINT SOURCE CAN
- 520 IF TH>900 THEN FR=SQR(TH/900) : REM APPEAR EXTENDED
- 530 FC=10^(0.4*(CI/2-1)) : REM COLOR OF STAR
- 540 FS=1.0 : REM OBSERVER'S SENSITIVITY
- 550 REM
- 560 REM CALCULATE SKY BRIGHTNESS
- 570 REM
- 580 IF MZ>=(7-K) THEN 620 : REM
- 590 XX=0.2*(8.68-K-MZ) : REM FS ASSUMED = 1
- 600 BS=39.7*(10^XX-1)^2 : REM SKY BRIGHTNESS FOR MZ
- 610 GOTO 650
- 620 BS=54 : REM BEST POSS. SKY BRIGHT-
- 630 FS=10^(0.4*(7-K-MZ)) : REM NESS & GOOD EYESIGHT
- 640 REM
- 650 BS=BS*(Z*Z*0.5+1) : REM ZENITH HAS DARKEST SKY
- 660 B=BS/(FB*FT*FPX*FA*FM*FC) : REM BACKGROUND BRIGHTNESS
- 670 REM IN TELESCOPE
- 690 REM CALCULATE LIMITING MAGNITUDE
- 700 REM
- 710 I=CC*(1+SQR(KK*B))^2 : REM Hecht (JOSA,v37,p59,1947)
- 720 IS=I*FB*FE*FT*FPX*FA*FR*FC*FS : REM FOR NO SCOPE, NO AIR
- 730 M=-16.57-2.5*LOG(IS)/LOG(10) : REM INTENSITY TO V MAG
- 740 M=M+(EX-6)*0.16 : REM EMPIRICAL EXPERIENCE
- 750 REM CORRECTION
- 760 PRINT "VISUAL LIMITING MAGNITUDE = ";M
- 770 END
- 800 REM
- 810 REM This program by Bradley Schaefer calculates the
- 820 REM limiting stellar magnitude an observer can expect
- 830 REM to see with various types and sizes of telescopes,
- 840 REM and under various conditions. It is fully discussed
- 850 REM in SKY & TELESCOPE magazine, November, 1989, page 522.
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