en:documentation:display_of_neos
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| en:documentation:display_of_neos [2017/02/17 18:21] – change by Basil Rowe pch | en:documentation:display_of_neos [2022/06/28 14:14] (current) – [New method since version 4.3] pch | ||
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| This method can only work for the flyby of a well know asteroid with a good precision for the circumstance of the flyby. This is necessary for the MPC or Horizon to compute a precise perturbed orbit.\\ | This method can only work for the flyby of a well know asteroid with a good precision for the circumstance of the flyby. This is necessary for the MPC or Horizon to compute a precise perturbed orbit.\\ | ||
| In the case of a newly discovered object it is better to use the other method [[# | In the case of a newly discovered object it is better to use the other method [[# | ||
| + | |||
| + | ===== New method since version 4.3 ===== | ||
| + | |||
| + | Since the beta version from February 2021 it is possible to compute the object position directly in the program using a SPICE kernel for the NEO (or other asteroid). Even for a perturbed orbit this method give the same precision than Horizon.\\ | ||
| + | It automate the Horizon Telnet interface to prepare a kernel file and download it by FTP. | ||
| + | |||
| + | Open Setup -> Solar System, then the tab **SPICE ephemeris** | ||
| + | |||
| + | The first time you need to enter your email that is required by JPL. Enter the name of the NEO, the first day you want the position, the number of days of the prevision. \\ | ||
| + | Do not enter a too long period here because this can increase the file size a lot, but also because the prevision is continuously updated with new observation that increase it's precision. It is easy to update the file later to extend it's validity.\\ | ||
| + | When ready click **Download**. | ||
| + | |||
| + | {{: | ||
| + | |||
| + | After the download is complete you see a new entry in the list below.\\ | ||
| + | Be sure to select the object you want to display on the chart.\\ | ||
| + | A mouse right click present a menu to refresh or delete one or all of the ephemeris.\\ | ||
| + | Click **OK** at the bottom of the window. | ||
| + | |||
| + | {{: | ||
| + | |||
| + | To locate the new object type the name in the search toolbar and press Enter. | ||
| + | |||
| + | {{: | ||
| + | |||
| + | The display of this object is independent of the asteroid that not need to be selected.\\ | ||
| + | There is also an independent selection available to plot the orbit path. | ||
| + | |||
| + | {{: | ||
| + | |||
| + | |||
| + | ---- | ||
| + | |||
| + | ===== Old method using local catalog ===== | ||
| It is possible to display Near Earth Objects (NEOs) in Skychart after meticulous calculation of their positions on the sky. To do these calculations, | It is possible to display Near Earth Objects (NEOs) in Skychart after meticulous calculation of their positions on the sky. To do these calculations, | ||
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| In case of NEOs, these normal conditions are not the case. To make predicitons about time and position, we need to do calculations based on three bodies: The object itself, the Sun and the Earth. Under the extra influence of Earths gravity, the track of the object does not follow its former conical section orbit anymore. Because orbital elements describe only conical sections, these aren't helpful in case of NEOs. If you would hold on to use orbital elements during a flyby event, you wil notice great changes of the orbital element data over short periods of time. Only after the object has moved far enough from Earth' | In case of NEOs, these normal conditions are not the case. To make predicitons about time and position, we need to do calculations based on three bodies: The object itself, the Sun and the Earth. Under the extra influence of Earths gravity, the track of the object does not follow its former conical section orbit anymore. Because orbital elements describe only conical sections, these aren't helpful in case of NEOs. If you would hold on to use orbital elements during a flyby event, you wil notice great changes of the orbital element data over short periods of time. Only after the object has moved far enough from Earth' | ||
| - | ===== Download of the CatGen project-files | + | ==== Download of the CatGen project-files ==== |
| You can use ephemerides calculations from both the Minor Planet Center (MPC) and the NASA JPL Horizons, or you can choose one of them. Skychart is capable to display catalogues of both sources in one single chart. \\ \\ | You can use ephemerides calculations from both the Minor Planet Center (MPC) and the NASA JPL Horizons, or you can choose one of them. Skychart is capable to display catalogues of both sources in one single chart. \\ \\ | ||
| For our convenience, | For our convenience, | ||
| Line 32: | Line 66: | ||
| | **README.txt** | Short description of the purpose of these files.| | | **README.txt** | Short description of the purpose of these files.| | ||
| - | First of all, download [[http://www.centaurus-a.nl/home/files/ | + | First of all, download [[https://ap-i.net/pub/skychart/neo/ |
| Unzip the file in your catalogue directory. After that, you will find a new directory named '' | Unzip the file in your catalogue directory. After that, you will find a new directory named '' | ||
| - | ===== Retrieval of Minor Planet Center data ===== | + | ==== Retrieval of Minor Planet Center data ==== |
| Open the source of the MPC data [[http:// | Open the source of the MPC data [[http:// | ||
| Select the radio button '' | Select the radio button '' | ||
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| If you don't want to use ephemerides data from Horizons you can savely skip the next paragraph and continue with [[en: | If you don't want to use ephemerides data from Horizons you can savely skip the next paragraph and continue with [[en: | ||
| - | ===== Retrieval of Horizons position data ===== | + | ==== Retrieval of Horizons position data ==== |
| Open [[http:// | Open [[http:// | ||
| Line 92: | Line 126: | ||
| Now open in the earlier created '' | Now open in the earlier created '' | ||
| - | ===== Generation of an ephemerides catalogue with CatGen | + | ==== Generation of an ephemerides catalogue with CatGen ==== |
| If you keep the default file name for the data and you not want to do any change to the provided example mpc.hdr or hori.hdr you can skip this section and go directly to [[display_of_neos# | If you keep the default file name for the data and you not want to do any change to the provided example mpc.hdr or hori.hdr you can skip this section and go directly to [[display_of_neos# | ||
| Line 125: | Line 159: | ||
| === Activate the catalogue === | === Activate the catalogue === | ||
| - | From the menu: **Setup → Catalog**, then the tab **Catalog** in the dialog, click at the button **Add** in order the tell Skychart where to find your new catalog. Search for the '' | + | From the menu: **Setup → Catalog**, then the tab **Catalog** in the dialog, click at the button **Add** in order the tell Skychart where to find your new catalog. Search for the '' |
| + | Also be sure Skychart is configured to show the Deep Sky Objects because the symbol used to draw the asteroid position are DSO symbol.\\ | ||
| ===== Display ===== | ===== Display ===== | ||
en/documentation/display_of_neos.1487352076.txt.gz · Last modified: 2017/02/17 18:21 by pch
