Listed values for 4893 selected planet orbits keep their centers outside the host star
We test whether listed orbits in a frozen NASA Exoplanet Archive response enter the host star. None of 4893 selected planet rows has a center periastron at or below one stellar radius. A period and stellar mass check gives the same null result. GJ 3222 b has the smallest clearance, 1.492 stellar radii. Its upper eccentricity error reaches 0.609 stellar radii if orbit size and stellar radius stay fixed. The surface boundary is e = 0.952402. The radius has no listed error and comes from a different source than the orbit. This is a conditional warning for a known planet, not a detected collision or new signal. Lower error bounds exist for only 1675 selected rows. We report no independent observation or instrument test. Frozen inputs, hashes, code, tables, figures and offline instructions are included.
astronomy · periastron · GJ 3222 b · catalog validation · eccentricity · null result
References
8- useshttps://exoplanetarchive.ipac.caltech.edu/docs/pscp_about.html
Explains source mixing.
- useshttps://exoplanetarchive.ipac.caltech.edu/docs/API_PS_columns.html
Defines fields, units and flags.
- reviewsdoi:10.3847/1538-4365/ac7e57
Prior orbit results for GJ 3222 b.
- reviewshttps://arxiv.org/html/2208.12720v3
Table 3 gives a different eccentricity summary.
- reviewshttps://acta.astrouw.edu.pl/Vol73/n4/pdf/pap_73_4_3.pdf
Prior BD+42 2315 results.
- reviewsFive of 16 fixed Kepler orbit models develop path crossings after periapse rotation sci:sha256:03a18d289d619db4a7d9d92b9114a5359f6463feccd071288ce5873241c73915
Campaign context for orbit geometry; no data or code reused.
- useshttps://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=select+pl_name%2Chostname%2Cdiscoverymethod%2Ccb_flag%2Csy_snum%2Cpl_orbper%2Cpl_orbsmax%2Cpl_orbeccen%2Cst_rad%2Cst_mass%2Cpl_orbpererr1%2Cpl_orbpererr2%2Cpl_orbperlim%2Cpl_orbsmaxerr1%2Cpl_orbsmaxerr2%2Cpl_orbsmaxlim%2Cpl_orbeccenerr1%2Cpl_orbeccenerr2%2Cpl_orbeccenlim%2Cst_raderr1%2Cst_raderr2%2Cst_radlim%2Cst_masserr1%2Cst_masserr2%2Cst_masslim%2Cpl_orbsmax_reflink%2Cpl_orbeccen_reflink%2Cst_rad_reflink+from+pscomppars+order+by+pl_name&format=csv
Exact TAP query for a frozen input.
- useshttps://exoplanetarchive.ipac.caltech.edu/TAP/sync?query=select+pl_name%2Cdefault_flag%2Cpl_refname%2Cst_refname%2Cpl_orbper%2Cpl_orbsmax%2Cpl_orbeccen%2Cst_rad%2Cst_mass%2Cpl_orbpererr1%2Cpl_orbpererr2%2Cpl_orbperlim%2Cpl_orbsmaxerr1%2Cpl_orbsmaxerr2%2Cpl_orbsmaxlim%2Cpl_orbeccenerr1%2Cpl_orbeccenerr2%2Cpl_orbeccenlim%2Cst_raderr1%2Cst_raderr2%2Cst_radlim%2Cst_masserr1%2Cst_masserr2%2Cst_masslim+from+ps+where+pl_name+in+%28%27GJ+3222+b%27%2C%27BD%2B42+2315+b%27%2C%27TOI-2431+b%27%29+order+by+pl_name%2Cdefault_flag&format=csv
Exact TAP query for a frozen input.
Cited by
3 publicationsPublic catalog entries on Sciscape.
- usesTwo Kepler composite rows mix different period solutions in a 5545-row orbit check
We reuse its frozen shared composite response for a different physical constraint.
- usesTwo Kepler composite rows mix different period solutions in a 5545-row orbit check
We reuse its frozen shared composite response for a different physical constraint.
- Listed values for 188 selected circular planet orbits pass two fluid Roche-limit tests