Planetary, Lunar, and Stellar Visibility represents an interesting means of showing users a 3-color diagram that represents when the moon, a star, a planet or the sun are visible during any year starting from 3000 BC to AD 6000 at any region on the planet The vertical axis marks the months of the year, the horizontal axis marks the hours of the day.
The three colors create a contour map effect and show whether the body is under the horizon (black) and invisible, above the horizon with the sun (light color) and invisible, above the horizon without the sun (shaded color) and so possibly visible.
The times of sunrise and sunset and when the sun reaches specified altitudes above or below the horizon can be shown as curves on the diagrams. By moving the mouse over the diagram, the date and time along with the object’s altitude, azimuth, and magnitude, or the phase of the moon, are displayed.
In addition, Planetary, Lunar, and Stellar Visibility computes and tabulates the dates of visibility phenomena: for planets and stars first and last visibility, acronychal rising and cosmical setting; for the moon first and last visibility, and the tables provide much supplementary information.
These phenomena are very useful for historical purposes. Since the computation of visibility phenomena is complex and uncertain, alternate methods are provided and parameters can be altered by the user to find what appear to be the best results.
There are also diagrams of solar and lunar eclipses, of the rotation, inclination, illumination, and apparent size of the bodies, and of Jupiter’s satellites. The settings for the computations may be saved, the graphics may be saved, pasted into documents, and printed, and the tables for visibility phenomena may be accumulated, edited, printed, and saved as .rtf files or HTML files to be pasted into documents and printed.
Provides:
visibility diagrams for the sun, moon, planets, and stars
dates of heliacal phenomena of planets and stars
dates of first and last visibility of the moon
.rtf files of all information for visibility phenomena
HTML files of times of rising, culmination, and setting of the sun and the moon, planet or star, with differences, for each day of the year
HTML files of all information for visibility phenomena for up to 100 years
documentation, which explains the program, methods of computation, and user modifications
Planetary, Lunar, And Stellar Visibility Free
Planetary, Lunar, and Stellar Visibility Full Crack (PLV) is a program that displays the three-color visibility diagrams of planets, the moon, and the sun and shows the times of first and last visibility of those bodies. This program also calculates the times of rising, culmination, and setting of the sun and the moon, the times of first and last visibility of the planets, the date of the equinox, and the dates of first and last visibility of stars.
This program is based on an algorithm of the times of astronomical phenomena that is very fast and accurate. Its CPU time is less than two hours on a typical desktop computer and less than one hour on a typical laptop computer. It runs on Microsoft Windows and Linux.
The program is divided into a set of classes and subclasses, one for each body in the Solar system. These classes contain a set of methods for their behavior and phenomena, including the computation of the dates of these phenomena. The methods compute, for example, the times of rising, culmination, and setting of the sun and the moon, the dates of first and last visibility of the planets, the dates of first and last visibility of the moon, the dates of the equinox, and the dates of first and last visibility of stars.
.rtf files of all information for visibility phenomena
HTML files of times of rising, culmination, and setting of the sun and the moon, planet or star, with differences, for each day of the year
HTML files of all information for visibility phenomena for up to 100 years
documentation, which explains the program, methods of computation, and user modifications
Documentation
This document describes the nature of the different types of diagrams for planets, the moon, and the sun, and shows the times of first and last visibility of these bodies.
This document contains a description of the algorithm of times of phenomena and dates of phenomena, which underlies the program, along with an explanation of the types of diagrams displayed.
The times of astronomical phenomena are computed and tabulated using the following methods:
For every day of the year, the times of sunrise, sunset, noon, sunset, and midnight are computed from the geographic longitude and latitude, and the solar declination and obliquity.
The times of noon are computed from these times and the sidereal time.
The days of the week are identified and the times of the week are identified.
The times of sunrise and sunset are identified, the dates of the equin
Planetary, Lunar, And Stellar Visibility With License Code 2022
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Planetary, Lunar, And Stellar Visibility Full Version [Win/Mac] (April-2022)
Planetary, Lunar, and Stellar Visibility is an excellent solar and planetary program, and can be considered a general astronomy program. It will give you solar and planetary positions and times, phases, magnitudes, diameters, and other information.
It is especially useful for timing purposes. It is simple to use and fast to run. It can tabulate the times of dawn, dusk, and astronomical twilight. It can compute astronomical and geographical twilight, and compute the times of illumination and horizon of the planets and stars for any time. Planetary and Lunar Visibility will calculate the times of the phases of the Moon for any date. With the program can be saved. Some information is used to produce excellent graphics of planets, moon, and stars. Planet and star positions and times can be saved as.rtf files.
The Moon and planets are shown in a 3-D display as circles, lines, or dots. Moon phases are shown as dots, squares, and circles. The phase of the moon and Moon positions and times are displayed in a 3-D display.
The data is tabulated into four windows. In the first window are the tables of times of rising, culmination, and setting for the Sun and the Moon. In the second window are the tables of phases of the Moon, Moon eclipses, and the Sun and the Moon in 3-D. In the third window is a graph that shows the phases of the Moon. In the fourth window is a graph that shows the positions of planets and the Moon. A “picker” allows the user to select any date, month, and year. Planetary and Lunar Visibility will also tabulate the times of sunrise and sunset, the dates of heliacal rising and setting of planets and stars, and the dates of first and last visibility of the Moon.
.rtf files of all information for visibility phenomena for up to 100 years
HTML files of all information for visibility phenomena for up to 100 years
.html files of all information for visibility phenomena for up to 100 years
Date range for the tables of heliacal phenomena of planets and stars, astronomical twilight, and geographical twilight:
year: 3000 BC to AD 6000
month:
day:
Invisibility Table for the Sun:
Month:
Year:
visible above the horizon:
sunrise and sunset dates and times for the Sun
visible without the sun:
sunrise and sunset dates and times for the Sun
Invisibility Table for the Moon:
Month
What’s New in the Planetary, Lunar, And Stellar Visibility?
Inflate the PDF image of the site to fully display the project description, license information, and the actual program.
A:
MTS: Moon, stars, sun, planet
Description:
Provides a graphical user interface (GUI) to the Moon, stars, sun, and planets.
Cost:
Free
A:
Open Source Astronomy
Description:
Generate an image of the moon, stars, sun, and planets, as seen from the viewer’s current location, at any time of day or night.
Cost:
Free
What is this?
Many free astronomy software packages exist which will produce a diagram of the sky. This free software however is different in that it is not a library of predefined diagrams of the sky. Instead it is a single program which is able to generate a diagram of the night sky as seen from any location on the planet.
Open Source Astronomy is:
A single program. It is not a library of diagrams. It has its own unique code base.
Adaptable for use with any location on the planet.
Uses interactive, real-time, on-the-fly computation. The program does not display a static diagram. It interacts directly with the user.
The user can easily generate diagrams for any location on the planet.
Provides many predefined diagrams of the night sky.
Saves the graphics files to local disk.
Configurable. Configure data types, resolution, and time ranges to suit your needs.
What can I do with it?
As stated above, the user can easily generate diagrams for any location on the planet. For example:
Use it to generate a daytime (sunup-sunset) diagram for any location on the planet.
Use it to generate a diagram of any planet or planetoid during a full moon.
Use it to generate a diagram of any planet or planetoid when it is at the same location relative to the Sun during a lunar eclipse.
The program also works with other bodies in the solar system:
Use it to generate a diagram of the Moon as it moves through its orbit.
Use it to generate a diagram of Jupiter’s Galilean satellites as they orbit the planet.
Use it to generate a diagram of Uranus’ moons as they orbit the planet.
Use it to generate a diagram of the “Littrow star” as it moves through the “Pioneer 11 shadow”.
Use it to generate a diagram of Saturn’s moons.
Use it to generate a diagram of Mars as it moves through its orbit.
Use it to generate a diagram of the planets in the solar system as they move through their orbits.
Can I save the graphics?
Yes. The user may save the output as a.gif,.jpg,.png,.bmp,.
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