In 1970 I designed 9* C.A. telescope for MSS Multi-Spectral-Scanner (depicted) that took 1st compleat photos of planet Earth (Photos in every Atlas, 30m res)
1st the Orion 4.5"C.A. is 114.3 mm (10,261mm*2) vs 90mm C.A. (6,362mm*2) for greater photon gathering Clear Aperture by factor of 1.61 or 61% more light but Larger dia (C.A.=Clear Aperture) also means higher RESOLUTION & that counts IF U want to see sharp edges of moon craters, saturn rings, etc
2nd Orion Starburst uses a Reflective Mirror that's also PARABOLIC so U get purrfect reflection to focus of distant objects, one step better than a spherical optic> A mirror has no color aberations whereas a Refractor glass lens will have some dispersion of different colors & color distortion> A Refractor lens is like a stack of prisms that bend light as if it were a rainbow to steer light onto focus, but slight differences in angle for eash "rainbow" light color leads to image distortion by smearing different colors off of point> A Reflecting Mirror has no such issues
That's why MSS was a reflecting telescope w/a parabolic primary but a shpherical secondary b/c its SECRET was the Semi-Kinematic Truss aimed its CENTROID at the center of radius of 2nd mirror> U could strike it w/a ball peen hammer and the 'scope would NOT DEFOCUS> Perkin Elmer Corp built the MSS telescope & told me it was the BEST they'd ever built b/c of that feature (PE built Hubble too)
Also noticed Orion has a 2X Barlow lens> sorta' a supercharger for amplifying the IMAGE U will observe from your basic F/4 telescope> F/4 means Focal length is 4 times C.A. or only 18" to keep scope length short b/c the image produced by the primary has to be in a position where your eyepiece can observe it> The MSS had a 4 foot (48") focal length so F/# was 48"/9"=F/5.3> Orion F./4 is a bit faster When they say "Fast" they mean the photons collected by C.A. R brought into focus quickly (shortened so U can get a compact telescope, but NOT too fast b/c U still want sharp resolution and that's another reason for a Reflector, it can be fast
So in closing, I'd take the ORION Reflector telescope that I surmise is a Newtonian design wherein primary reflects a sharp image up to a flat mirror that folds the image beam out towards the eyepiece for viewing>
I built a Dobsonian 10"C.A. Side Walk Astronomer telescope in 1994 w/a 69" focal length that I later "Stopped Down" to 8"dia. by laying an auto air clnr on top of primary> (For backyard astronomy 10" C.A. is cost-effective size limit) Used a Sona-Tube concreate tube for main hsg and in pollishing the mirror the SECRET is in final stages of fine grit, put a 4" FOAM slab over polishing tool & lay a 7.5 lb weight on top of the foam for PURRFECT pressure on to do polish
U can measure F.L. by shining a flashlight into your scope from a distance & holding a piece of white paper next to the flashlight & move towards telescope until flashlight IMAGE on paper exactly matches REAL flashlight & then U R at twice the focal length> U can measure it w/in a fraction of an inch if U nudge it
In 1979 I published a paper in Machine Design on Simplified Optics wherein I used dimensional analysis to combine Paraxial Equations of Optics into only 2 equations> Image location & Magnification> It shows 1 to 1 magnification at 2 focal lengths> Gave it to "Bible of Optics" by Melles Griot, they loved it & used it to expand into laser beams> Give me an email address & I'll send a copy
Cordially,
Roger E Carmichael, BSME
Man, the MSS design was 50yrs ago> Never told anyone its secret 'till now b/c during the Cole War we had to keep the lid on it lest Commies get ahold of it