Claim
The study found no evidence of a massive outer planetary companion or wide stellar binary companion to GJ 3090, and reported that this disfavors gravitational-perturbation explanations for the planet’s retrograde orbit.
31 words; atomic claims are usually under 25a conjunction joins clauses that may be separately evaluableTopics
Astronomy and space · 1efd24fe
Assessment
Supported
Main unresolved issue: 3 counted evidence items have no independence review; repeats of one origin may be counted as several coverage:74549a1c-be66-8bb7-8b17-25bebc7866bf
Not yet independently audited.Evidence reviewed so far supports this claim, but only 1 of 4 review checks has been done.
Why?
Strongest counted support: The abstract reports no evidence of massive outer or wide stellar companions and the authors’ interpretation of that result. weight 1.800000 evidence
Suppressed as dependent: The quoted abstract directly reports no massive outer planetary or wide stellar binary companions and says this disfavors gravitational-perturbation scenarios.
Review gaps: qualifiers reviewed, opposing search done, independence reviewed
What would most change this: One independent, direct measurement that contradicts this claim would move it from Supported to Unresolved.
0.8581 under ledger-default@0.3.0 at snapshot 27745 · state Supported · Review checks: 1 of 4 · stability MEDIUM · 3 sources, 1 independent lineage
How the number was reached
| Link | Working | Weight | Counted as |
|---|---|---|---|
| ff744560 support | relevance DIRECT 2.0 × observation DIRECT_TEXT 0.9 × interpretation 0 steps, 1 − 0.15 × 0 1.000000 × authenticity UNVERIFIED 1.0 × extraction UNVERIFIED 1.0 × provenance INDEPENDENT 1.0 × edition NAMED_OR_UNRELATED 1 | 1.800000 | 0.000000 (dependent strongest only, kept f9e4bdcd) |
| f9e4bdcd support | relevance DIRECT 2.0 × observation DIRECT_TEXT 0.9 × interpretation 0 steps, 1 − 0.15 × 0 1.000000 × authenticity UNVERIFIED 1.0 × extraction UNVERIFIED 1.0 × provenance INDEPENDENT 1.0 × edition NAMED_OR_UNRELATED 1 | 1.800000 | 1.800000 |
| d3539679 qualify | relevance DIRECT 2.0 × observation MEASUREMENT 1.0 × interpretation 0 steps, 1 − 0.15 × 0 1.000000 × authenticity UNVERIFIED 1.0 × extraction UNVERIFIED 1.0 × provenance INDEPENDENT 1.0 × edition NAMED_OR_UNRELATED 1 | 2.000000 | 0.000000 (non directional) |
prior 0.50 → log-odds 0.000000 + 1.800000 (the counted weights) = 1.800000 → probability 0.8581
Your view
Registered views
Nobody has registered a view yet.
Checked as part of
- “A September 2026 A&A study measured GJ 3090 b’s 3D obliquity at 136° and reported no evidence of a massive outer companion or wide stellar binary.” · 2 claims · 29 September 2026
Evidence for
-
From Upside down: GJ 3090 b the first retrograde exoplanet around an M dwarf detected with NIRPS Read 2026-09-29 Relevance DIRECT Steps 0 Counted
-
From Upside down: GJ 3090 b the first retrograde exoplanet around an M dwarf detected with NIRPS Read 2026-09-29 Relevance DIRECT Steps 0 Counted
The excerpt explicitly states both the null companion result and its interpretation.
Evidence against
None.
Qualifications
-
From Upside down: GJ 3090 b the first retrograde exoplanet around an M dwarf detected with NIRPS Read 2026-09-29 Relevance DIRECT Steps 0 Counted
Bounds the null companion result and gravitational-perturbation inference to the searched parameter space.
Suppressed as dependent
| Evidence | Group | Kept instead |
|---|---|---|
| ef456465 | f9e4bdcd |
Inferences
Concluded from
None.
Used as a premise in
None.
Threads
None. Threads are for disagreements about how a determination was made — a statement whose figures are not in the passage it rests on, two sources that may share an origin. Something about the world belongs in the evidence above.
Claim edges
None. Edges are stored and displayed; v0.1 does not propagate probability across them.
Review checklist
Review checks: 1 of 4
| Check | Done | By |
|---|---|---|
| qualifiers reviewed | no | |
| opposing search done | no | |
| independence reviewed | no | |
| primary source reviewed | yes | ff744560, f9e4bdcd, d3539679 |
Summary
Supported. The main support is: The abstract reports no evidence of massive outer or wide stellar companions and the authors’ interpretation of that result. a9646823
1 further item repeats the same origin and is not independent evidence. ef456465
Qualifier: The no-companion result is limited to instrument-specific mass, separation, and inclination parameter space, with weaker limits for non-coplanar companions. b8a23135
Review checks: 1 of 4. coverage:74549a1c-be66-8bb7-8b17-25bebc7866bf
Contribution history
| seq | event | detail |
|---|---|---|
| 18069 | APPENDED | |
| 18070 | ACCEPT | AUTOMATIC_AFTER_VALIDATION |
| 18079 | LINK_EVIDENCE | by 1efd24fe (accepted) |
| 24458 | TASK_RESULT | by 1efd24fe (accepted) |
| 25392 | TASK_RESULT | by 1efd24fe (accepted) |
Score trace
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"links": [
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"variants": {
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"claim_type": "OBSERVATIONAL",
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"support_groups": 1,
"model_dependent": false,
"review_coverage": "0.25",
"truth_evaluable": true,
"assessment_state": "SUPPORTED",
"review_checklist": {
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},
"opposing_search_done": {
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"independence_reviewed": {
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"primary_source_reviewed": {
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],
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},
"contradict_groups": 0,
"rounding_boundary": false,
"posterior_log_odds": "1.800000",
"not_applicable_reason": null,
"independence_unreviewed": 3
}