Deep-Sky Planner Help
Deep-Sky Planner Help

 

 

Navigation: Deep-Sky Planner Help > Appendix >

Visibility Modeling

 

 

 

 

Visibility Modeling

Deep-Sky Planner includes mathematical models that predict whether an object can be seen, given a set of equipment and sky conditions. In the case of extended deep-sky objects and single stars, it means whether the object can be detected visually. In the case of a double star, this means whether the pair can be split visually.

These models are the product of several years of research and field testing by the author, and published research by other scientists. These models are intended to provide guidance rather than an absolute answer to the question of whether an object can be seen.

The models require various input parameters in addition to object data. The table below describes the data required by the various models. Important: A model cannot be employed if any of the required input data are missing. Some of the input parameters are objective in nature while a few are rather subjective. If the visibility model is yielding results that seem incorrect given instrument, observer and sky conditions, these subjective parameters might be adjusted for improved results. In particular, you might adjust (in the order of greatest significance): observer's experience level, instrument's cleanliness or observer's dark-adapted eye pupil size.

Object Type

Sky Conditions Required

Equipment/Observer Information Required

Extended Deep-Sky Objects, Larger Planets

Darkness and transparency

Instrument aperture, optical system transmission, eyepiece apparent field or binocular true field, dark-adapted eye pupil size

Double Stars

Seeing

Instrument aperture, obstruction (if any) and cleanliness (if any), observer's dark-adapted eye pupil size and experience level

Single Stars, Carbon Stars, Asteroids, Smaller Planets

 

Instrument aperture and cleanliness (if any), observer's dark-adapted eye pupil size and experience level

Variable Stars

 

Instrument aperture and cleanliness (if any), observer's dark-adapted eye pupil size and experience level

The result of the models' computations are shown below. These results appear on reports in the Vis Model column.

Object Type

Vis Model

Comments

Extended Deep-Sky Objects, Larger Planets

 

Easy

The object is bright enough to be seen without difficulty.

 

Moderate

The object is bright enough to be seen with some difficulty.

 

Difficult

The object may be bright enough to be seen. Try to observe this object at its highest altitude in the sky at a dark location, and be sure to use averted vision.

 

Improbable

The object is probably too dim to be seen. Try to observe this object at its highest altitude in the sky at a dark location.

 

Too dim

The object is too dim to be seen.

 

Too low

The object is low in the sky; the model becomes very inaccurate at low altitudes.

 

Down

The object is below the horizon

 

<blank>

The object can't be modeled due to missing data.

Double Stars

 

Easy

Both stars in the pair are bright enough to be seen, and they may be resolved. The two stars appear to be widely separated.

 

Moderate

Both stars in the pair are bright enough to be seen, and they may be resolved. The two stars may appear to be fairly close, but they appear to be clearly separated.

 

Difficult

Both stars in the pair are bright enough to be seen, and they may be resolved. The two stars may appear to be touching or they may be separated by a hair-line gap.

 

Improbable

Both stars in the pair are bright enough to be seen but the pair is so close that it is improbable that they can be resolved. The two stars may appear to be a rod-shaped or figure-8 shaped star.

 

No split

Both stars in the pair are bright enough to be seen but the pair is too close to be resolved.

 

Sec. dim

The primary is bright enough to be seen but the secondary is not.

 

Both dim

Both stars in the pair are too dim to be seen.

 

Unmodeled

The stars fall outside the modeled parameters.

 

Down

The stars are below the horizon

 

<blank>

The stars can't be modeled due to missing data.

Single Stars, Carbon Stars, Asteroids, Smaller Planets

 

Visible

The object is bright enough to be seen.

 

Too dim

The object is too dim to be seen.

 

Down

The object is below the horizon

 

<blank>

The object can't be modeled due to missing data.

Variable Stars

 

Visible

The star is bright enough to be seen throughout its magnitude range.

 

Maybe

The star may be seen when it is at its brightest magnitude, but not at its dimmest magnitude; thus, it may be visible depending on where it is in its light curve.

 

Too dim

The star is too dim to be seen even when it is at its brightest magnitude.

 

Down

The star is below the horizon

 

<blank>

The star can't be modeled due to missing data.

 

 


 

Help file version 9.2.3.0 ▪ Copyright © 2024-2026 Knightware, LLC

 

 

 

Help file version: 9.2.3.0  Copyright © 2026 Knightware, LLC