Check if a Solar System object is (or was) observable by NASA's K2 mission. This command will query JPL/Horizons to find out.
Project description
# K2ephem [![PyPI](http://img.shields.io/pypi/v/K2ephem.svg)](https://pypi-hypernode.com/pypi/K2ephem/) [![PyPI](http://img.shields.io/pypi/dm/K2ephem.svg)](https://pypi-hypernode.com/pypi/K2ephem/) [![Travis status](https://travis-ci.org/KeplerGO/K2ephem.svg)](https://travis-ci.org/KeplerGO/K2ephem) [![DOI](https://zenodo.org/badge/doi/10.5281/zenodo.44363.svg)](http://dx.doi.org/10.5281/zenodo.44363)
***Checks whether a Solar System body is (or was) observable by [NASA's K2 mission](http://keplerscience.arc.nasa.gov).***
[NASA's K2 mission](http://keplerscience.arc.nasa.gov) is using
the unique assets of the repurposed Kepler space telescope
to perform long-baseline, high-cadence, high-precision photometry
of targets selected by the community.
Unlike the original Kepler mission, the loss of two reaction wheels
requires K2 to point near the ecliptic plane.
As a result, K2 can provide high-precision lightcurves
for large numbers of asteroids, comets, and (dwarf) planets.
This repository provides a command-line tool that uses the JPL/Horizons
service to check whether a Solar System body is (or was) in the footprint
of one of the past or future [K2 Campaign fields](http://keplerscience.arc.nasa.gov/k2-fields.html).
## Installation
You need to have a working version of Python installed.
If this requirement is met, you can install the latest stable version
of `K2ephem` using pip:
```
$ pip install K2ephem
```
If you have a previous version installed, you can upgrade it using:
```
pip install K2ephem --upgrade
```
Or you can install the most recent development version
from the git repository as follows:
```
$ git clone https://github.com/KeplerGO/K2ephem.git
$ cd K2ephem
$ python setup.py install
```
The `setup.py` script will automatically take care of installing two required dependencies (`K2fov` and `pandas`).
## Usage
After installation, you can call `K2ephem` from the command line.
For example, to verify whether comet *Chiron* can be observed by K2,
simply type:
```
K2ephem Chiron
```
Or you can type `K2ephem --help` to see the detailed usage instructions:
```
$ K2ephem --help
usage: K2ephem [-h] [--first campaign] [--last campaign] [-p] target
Check if a Solar System object is (or was) observable by NASA's K2 mission.
This command will query JPL/Horizons to find out.
positional arguments:
target Name of the target. Must be known to JPL/Horizons.
optional arguments:
-h, --help show this help message and exit
--first campaign First campaign to check (default: 0)
--last campaign Final campaign to check (default: 18)
-p, --plot Produce plot showing the object position with respect to
each campaign.
```
## Background
The [JPL/Horizons](http://ssd.jpl.nasa.gov/horizons.cgi)
ephemeris service allows users to predict the position
of Solar System bodies in the sky as seen from the Kepler/K2 spacecraft.
This can be achieved by entering `@-227` as the "Observer Location".
Setting the location to be the Kepler spacecraft is *crucial*,
because Kepler is more than 0.5 AU away from the Earth!
## Attribution
Created by Geert Barentsen for the NASA Kepler/K2 Guest Observer Office.
If this tool aided your research, please cite it using the [DOI identifier](http://dx.doi.org/10.5281/zenodo.44363)
or the following BibTeX entry:
```
@misc{geert_barentsen_2016_44363,
author = {Geert Barentsen},
title = {K2ephem: v1.1.1},
month = jan,
year = 2016,
doi = {10.5281/zenodo.44363},
url = {http://dx.doi.org/10.5281/zenodo.44363}
}
```
***Checks whether a Solar System body is (or was) observable by [NASA's K2 mission](http://keplerscience.arc.nasa.gov).***
[NASA's K2 mission](http://keplerscience.arc.nasa.gov) is using
the unique assets of the repurposed Kepler space telescope
to perform long-baseline, high-cadence, high-precision photometry
of targets selected by the community.
Unlike the original Kepler mission, the loss of two reaction wheels
requires K2 to point near the ecliptic plane.
As a result, K2 can provide high-precision lightcurves
for large numbers of asteroids, comets, and (dwarf) planets.
This repository provides a command-line tool that uses the JPL/Horizons
service to check whether a Solar System body is (or was) in the footprint
of one of the past or future [K2 Campaign fields](http://keplerscience.arc.nasa.gov/k2-fields.html).
## Installation
You need to have a working version of Python installed.
If this requirement is met, you can install the latest stable version
of `K2ephem` using pip:
```
$ pip install K2ephem
```
If you have a previous version installed, you can upgrade it using:
```
pip install K2ephem --upgrade
```
Or you can install the most recent development version
from the git repository as follows:
```
$ git clone https://github.com/KeplerGO/K2ephem.git
$ cd K2ephem
$ python setup.py install
```
The `setup.py` script will automatically take care of installing two required dependencies (`K2fov` and `pandas`).
## Usage
After installation, you can call `K2ephem` from the command line.
For example, to verify whether comet *Chiron* can be observed by K2,
simply type:
```
K2ephem Chiron
```
Or you can type `K2ephem --help` to see the detailed usage instructions:
```
$ K2ephem --help
usage: K2ephem [-h] [--first campaign] [--last campaign] [-p] target
Check if a Solar System object is (or was) observable by NASA's K2 mission.
This command will query JPL/Horizons to find out.
positional arguments:
target Name of the target. Must be known to JPL/Horizons.
optional arguments:
-h, --help show this help message and exit
--first campaign First campaign to check (default: 0)
--last campaign Final campaign to check (default: 18)
-p, --plot Produce plot showing the object position with respect to
each campaign.
```
## Background
The [JPL/Horizons](http://ssd.jpl.nasa.gov/horizons.cgi)
ephemeris service allows users to predict the position
of Solar System bodies in the sky as seen from the Kepler/K2 spacecraft.
This can be achieved by entering `@-227` as the "Observer Location".
Setting the location to be the Kepler spacecraft is *crucial*,
because Kepler is more than 0.5 AU away from the Earth!
## Attribution
Created by Geert Barentsen for the NASA Kepler/K2 Guest Observer Office.
If this tool aided your research, please cite it using the [DOI identifier](http://dx.doi.org/10.5281/zenodo.44363)
or the following BibTeX entry:
```
@misc{geert_barentsen_2016_44363,
author = {Geert Barentsen},
title = {K2ephem: v1.1.1},
month = jan,
year = 2016,
doi = {10.5281/zenodo.44363},
url = {http://dx.doi.org/10.5281/zenodo.44363}
}
```
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