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Lemmon A6 18 ottobre 2025

Lemmon A6 18 ottobre 2025

C/2025 A6 (Lemmon) is a non-periodic comet discovered by the Mount Lemmon Survey in images obtained on 3 January 2025. It has an inbound orbital period of about 1,350 years and will pass perihelion on 8 November 2025 when it will be 0.53 AU (79 million km; 49 million mi) from the Sun. This perihelion passage will reduce the orbital period to about 1,150 years.

SVBONY SV555 Astrograph Telescope APO - SV260 Astrophotography Filter.jpg

SVBONY SV555 Astrograph Telescope APO - SV260 Astrophotography Filter.jpg

SVBONY SV555 Astrograph Telescope APO - SV260 Astrophotography Filter.jpgSVBONY SV555 Astrograph Telescope APO - SV260 Astrophotography Filter.jpg

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Brand SVBONY
Model SV555
Aperture 54mm
Net Weight 2450g (excluding accessories)
Focal Length 243mm
Lens Coating Fully Multi Coated
Focuser Helical
Image Circle Φ 44mm (Full Frame)
Lockable 360º Rotator Yes
Objective Type Petzval Design(5 Elements in 3 Groups)
Optic Coated FMC
Mount Type Dovetail Plate
Dovetail Plate Length 184mm
Dovetail Plate Width 42mm
Lens Barrel Circumference 293mm
Front Filter Thread M72
Back-end connection M48x0.75 male thread
Length of Screws 2 x M6 short screws, length 10mm 2 x M6 long screws, length 55mm 2 x M4 screws, length 8mm 4 x M5 screws, length 12mm
Focal Ratio f/4.5-f/22


Brand

SVBONY

Model

SV260

Name

Multi-Broadband Filter

Size

2-inch

Substrate Thickness

2mm

Clear Aperture

44mm

Wavelength Range

300-1000nm

Blocking

>OD4@350-400nm; >OD2@Hg 589nm; >OD2@Hg 435.8nm; >OD2@Na 589.6nm; >OD1@Hg 546.1nm; >OD2@Na.615.4nm; >OD3@Hg 577nm; >OD2@Na.616.1nm; >OD3@Hg 578.1nm; >OD4@720-1100nm

Peak Transmittance

90%

Surface Quality

60/40

Surface Parallelism

1/2λ

Thread

M48x0.75

Single Thread

Yes

Net Weight

12.5g / 0.44oz /0.027lb

    1. Feature

    2. 1.5-band filter captures light across a broader spectrum; Accurately reproduces the true colors of celestial objects;
      2.Multi-Broadband filter properly designed for starfield shooting and deep sky photography, enhance stars and celestial bodies details; making deep sky observations clearer;
      3.Over 90% peak transmittance;reduces light loss, boasts an SII-OIII-SII band average transmittance of over 85%; Enhances contrast between the target object and the background;
      4.300-1000nm wavelength working range; multi-bandpass filter effectively combats light pollution; providing a broader coverage area;
      5.Max OD4 cut-off depth; astrophotography filters effectively block out unnecessary light; and provide stronger light pollution suppression.

Telescopes

SV555_User_Manual
1.31 MB pdf

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