More planets in 55 Cancri?
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Re: More planets in 55 Cancri?
Dnoces wrote:What's this systemic thing that I keep hearing about?
Systemic Console is a JAVA program to search extrasolar planets with available radial velocity data.
Take a look here:
http://207.111.201.70/php/viewdatabase.php?choice=real
And scrolling down you'll find a link "downloadable console". It's almost easy to use and can be executed without installation.

Edasich- Saturn-Mass

- Number of posts: 489
Age: 25
Location: Tau Ceti d - Northern hemisphere
Registration date: 2008-06-02

Re: More planets in 55 Cancri?
Thanks, I'm downloading it know.
Sure looks cool
Sure looks cool

Dnoces- Hydrogen Atom

- Number of posts: 4
Registration date: 2009-04-26
Re: More planets in 55 Cancri?
And if you have also radial velocity sets for "non-exoplanet-host" stars you can try searching for yet "unseen" planets =P

Edasich- Saturn-Mass

- Number of posts: 489
Age: 25
Location: Tau Ceti d - Northern hemisphere
Registration date: 2008-06-02

Re: More planets in 55 Cancri?
Additional planets can't be ruled out. However, constraints can be set in terms of the masses of additional planets in the system.
For the region between 55 Cancri f and 55 Cancri d, no planet can be larger than about 7 Mearth, or the planet would have been discovered by now. There is already a sufficient amount of radial velocity data to make it possible to find a super-Earth in the region if it exists.
For the region exterior to 55 Cancri d, the area of stability starts at around 10 au. Any planet larger than 40 Mearth in the region out to 15 au from the star would have revealed its presence through a long-term radial velocity trend. So far, there is no radial velocity drift to indicate the presence of additional planets in the 55 Cancri system.
For the region between 55 Cancri f and 55 Cancri d, no planet can be larger than about 7 Mearth, or the planet would have been discovered by now. There is already a sufficient amount of radial velocity data to make it possible to find a super-Earth in the region if it exists.
For the region exterior to 55 Cancri d, the area of stability starts at around 10 au. Any planet larger than 40 Mearth in the region out to 15 au from the star would have revealed its presence through a long-term radial velocity trend. So far, there is no radial velocity drift to indicate the presence of additional planets in the 55 Cancri system.
AVBursch- Hydrogen Atom

- Number of posts: 4
Registration date: 2009-05-01
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