2M 2140+16
The planetary system 2M 2140+16 hosts at least one planet.
| System parameters | |
|---|---|
| Name | 2M 2140+16 |
| Right ascension | 21h 40m 29s |
| Declination | +16° 25' 18" | Distance [parsec] | 25 | Distance [lightyears] | 81.5 | Number of stars in system | 1 | Number of planets in system | 1 |
Architecture of the system
This list shows all planetary and stellar components in the system. It gives a quick overview of the hierarchical architecture. 2M 2140+16 is not binary system, so the architecture is rather simple.
2M 2140+16, stellar object
2M 2140+16 b, planet, semi-major axis: 3.53 AU
Planets in the system
This table lists all planets in the system 2M 2140+16. If a row is empty, no data is available
| 2M 2140+16 b | |
|---|---|
| Alternative names | |
| Description and Trivia | |
| Lists | Confirmed planets |
| Mass [MJup] | 20 |
| Mass [MEarth] | 6357.8 |
| Orbital period [days] | 7340 |
| Semi-major axis [AU] | 3.53 |
| Eccentricity | 0.26 |
| Radius [RJup] | 0.92 |
| Radius [REarth] | 10.095344 |
| Temperature [K] | |
| Discovery method | imaging |
| Discovery year | 2010 |
| Last updated [yy/mm/dd] | 12/01/20 |
Stars in the system
This table lists all stars in the system 2M 2140+16. If a row is empty, no data is available
| 2M 2140+16 | |
|---|---|
| Alternative names | |
| Mass [MSun] | 0.08 |
| Radius [RSun] | 0.1 |
| Age [Gyr] | |
| Metallicity [Fe/H] | |
| Spectral type | |
| Temperature | 2300.0 |
| Visual magnitude |
Visualizations
Orbits
Planet sizes
The following plot shows the approximate sizes of the planets in this system The Solar System planets are shown as a comparison. Note that unless the radius has been determined through a transit observation, this is only an approximation (see Lissauer et al. 2011b).
Habitable zone
The following plot shows the approximate location of the planets in this system with respect to the habitable zone (green) and the size of the star (red). This is only an estimate, using the star's spectral type and mass. Note that if no green band is shown in the plot, then the planet's orbit is far outside the habitable zone. The equations of Selsis, Kasting et al are used to draw the inner and outer boundaries.
Scientific references and contributors
Links to scientific papers and other data sources
The following table lists all links which are relevant to this particular system.
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Note that this is just a summary. More references to the scientific publications and comments can be found in the commit messages. To see these, head over the github or click here to directly go to the git blame output of this system. In the left column of the output you can see the commit message corresponding to each parameter. It also lists the date of the last commit and the person making the changes. Within the commit message, you will find a link to the scientific publication where the data is taken from. Note that this is a new feature and not all system parameters might have a reference associated with it yet. Please help making this catalogue better and contribute data or references!
Open Exoplanet Catalogue contributors
This table lists all people who have contributed to the Open Exoplanet Catalogue. Please consider contributing! Click here to find out how.
| Number of commits | Contributor | |
|---|---|---|
|
|
Hanno Rein | hanno(at)hanno-rein.de |
View all commits contributing to the file 2M 2140+16.xml.
Data download
Click here to download the XML file for this system. It is part of the Open Exoplanet Catalogue. All information on this page has been directly generated from this XML file. As an alternative to the single XML file, you can also download the entire catalogue on github at https://github.com/hannorein/open_exoplanet_catalogue/. You can also find ASCII tables of the same catalogue at https://github.com/hannorein/oec_tables/. Some information, especially in the case of a binary system cannot be easily represented in an ASCII table. You are therefore encouraged to use the original XML files provided by the Open Exoplanet Catalogue.
Corrections
If you spot an error or if you can contribute additional data to this entry, please send an e-mail to exoplanet@hanno-rein.de. If possible, please include the corrected XML file of this entry and a reference to where the new data is coming from, ideally a scientific paper. If you are fluent with git and github, you can also create a pull request or open an issue on the Open Exoplanet Catalogue repository. In that case, your contribution will be properly attributed. Please include the reference in your commit message.