NEO Planner V5.0  -  Common restrictions  -  Explanations


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Within the picture, click on the zone that you want to be explained: (not in all browsers available)

These settings are the fifth step in getting NEO Planner up and running.  

Here you define some general constraints for the planning process.
These settings are primarily used to define the observable area in all directions from the observatory location, including self-defined lunar distances.
One should keep an eye on a horizon that is not too deep, even if the observatory allows this.


A full range from R.A. 12 east and west of the meridian makes it difficult for the program
to determine the best observation time for all objects, which is calculated based on the altitude of the nocturnal ephemeris.
So you should generally choose an area that is about 8-10 R.A. hours east or west of the meridian on midnight or more precisely, of the siderial time.

This range can be increased to a greater extent if one carefully checks the results of the calculations for correct chronological order.

Plausibility checks or actions are usually only carried out after leaving the cursor in the input field.

IAU Observatory Code:

The active observatory is displayed

- Moon restrictions

In contrast to deep sky photographers, the moon does not represent a real obstacle for observers of near-Earth objects.
Nevertheless, observation too close to our companion often leads to unusable images.

This is especially true for moon phases around 100%.
In this window you have the option to set the distances
between the objects and the moon depending on the phase based on your own experience.

Neo Planner then sorts out the objects whose positions are too close to the moon by the entered number of degrees during the night.
Experience has shown that when planning for moonlight, you should also set the maximum brightness of the objects lower.
 -> look here how to control the brightness of the objects

 

RA hours east before Siderial time:

Enter the RA hours which objects should be observed east of sidereal time depending on the nature of the horizon.
If the value is too small, there is a risk that objects that come close to the meridian during the night will not appear in the planning!

RA hours west after Siderial time:

Enter the RA hours which objects should be observed west of sidereal time  depending on the nature of the horizon.

 

 

Twilight end after sunset:

Light conditions on/off:

Display of the light conditions via a list box. At higher latitudes in the hemispheres,
reduced data is shown around the time of the summer solstice and missing astronomical time.
The twilight end and start times in the period between sunset and around nautical twilight should be adjusted to the seasons.

With this setting you define the time span between sunset and the start of the observation.
Since the start of the observation is based on individual experiences and preferences, enter the time span here yourself.
This can change during the year, depending on the location of the observatory.
For K87 on 50 degree northern latitude, I start the observation according to the sensitivity of my CCD camera, when nautical dusk is reaching MPSAS ~ 20 mag.
I then adjust the time span in the course of the year according to the seasons.

Twilight start before sunrise:

With this setting you define the time span between the last observation of the night and sunrise.
Since the end of the observation is based on individual experiences and preferences, enter the time span here yourself.
This can change during the year, depending on the location of the observatory.
For K87 on 50� northern latitude, I end the observation according to the sensitivity of my CCD camera, when nautical dusk is reaching MPSAS ~ 20 mag.
I then adjust the time span in the course of the year according to the seasons.

MPSAS -  Magnitude per Square Arc Second -  explanation

Minimum altitude ALT in degree:

The minimum height above the horizon depends primarily on experience as to which objects can reasonably be observed above the horizon with the equipment.
Near Earth Objects in particular require a high quality survey, so a generous degree value should be preferred.

Neo Planner then selects those objects which reach the specified height when crossing the meridian.

 

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Copyright: The author of NEO Planner and all sites of this web is Bernhard Haeusler, Dettelbach, Germany, all rights reserved