Galedra
Sign in Sign up

Claim

MeerKAT observations reported the first direct detection of auroral radio emission from the giant exoplanet β Pictoris b, including rapid recurring circularly polarized bursts and persistent emission from 0.85 to 3.5 GHz.

Type OBSERVATIONAL · truth-evaluable: yes · status at snapshot: ACTIVE · created seq 18097 · qualifiers {"location":"The giant exoplanet β Pictoris b observed with the MeerKAT array.","denominator":"Reported radio emission between 0.85 and 3.5 GHz."}

32 words; atomic claims are usually under 25a conjunction joins clauses that may be separately evaluable

Referenced 82 times: checked 2, looked up by assistants 0, viewed 52, shared 28. A count of attention, not evidence.

Topics

Astronomy and space · 1efd24fe

Assessment

Supported

Score: 0.9781 under ledger-default@0.3.0 at snapshot 27745

2 of 4 review checks done · 1 counted · 1 by the author only

2 independent evidence lineages · review checks 1 of 4 · stability HIGH

Main unresolved issue: 6 counted evidence items have no independence review; repeats of one origin may be counted as several coverage:f4f2064d-4398-8034-95c1-576288fae2cf

Not yet independently audited.Evidence reviewed so far supports this claim, but only 1 of 4 review checks has been done.A quoted passage from tech.cnr.cn was not found on the page when Galedra fetched it.

Why?

Strongest counted support: The abstract reports first direct exoplanet auroral radio detection with recurring polarized bursts from 0.85 to 3.5 GHz. weight 2.000000 evidence

Suppressed as dependent: The quoted passage directly reports the first direct exoplanet auroral radio detection from β Pictoris b, recurring circularly polarized bursts, and persistent emission at 0.85–3.5 GHz.

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 Supported.

Show calculation

Your view

Sign in to register whether you agree or disagree. A view is yours alone and never changes the assessment.

Registered views

Nobody has registered a view yet.

Registered views are personal belief, not evidence: they never change Galedra's assessment. Affiliations are self-declared and shown only for groups of 5 or more.

Checked as part of

Statements this claim was broken out of. The claim is scored on its own; a statement's reading only counts its claims.

Evidence for

Evidence against

None.

Qualifications

Suppressed as dependent

EvidenceGroupKept instead
0f881e4e0f80cc5d

Inferences

Concluded from

None.

Used as a premise in

None.

An inference is interpretation, not evidence: it never changes the assessment of its conclusion. Each premise is a claim with its own evidence.

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

2 checks by this claim's own author, alongside the independent review above. 1 QUALIFIER CHECK · 1 EVIDENCE VERIFICATION. A check by the person who recorded a claim does not raise its review coverage.

CheckDoneBy
qualifiers reviewedno
opposing search doneno
independence reviewedno
primary source reviewedyes4d9ed778, 740de84e, 0f80cc5d, b20be2c6, 29ff5699

Summary

Supported. The main support is: The secondary report says MeerKAT radio emission was localized to β Pictoris b rather than its host star and attributed to auroral activity. 59991feb

1 further item repeats the same origin and is not independent evidence. 0f881e4e

Qualifier: The 3.5 GHz upper endpoint is the top of the observing band, and the associated field estimate is a lower limit at the emission site. 4ef40f08

Qualifier: The reported detection is based on four MeerKAT observing occasions spanning 2025–2026 and the 0.8–3.5 GHz L/S bands. ffd68cfb

Qualifier: Recurring polarized bursts and persistent emission were observed, but rapid variability was not measurable in all epochs because of per-bin signal-to-noise limitations. 1f87d022

Review checks: 1 of 4. coverage:f4f2064d-4398-8034-95c1-576288fae2cf

Generated by stub-v0.1; every sentence cites graph ids.

Contribution history

seqeventdetail
18097APPENDED
18098ACCEPTAUTOMATIC_AFTER_VALIDATION
18109LINK_EVIDENCEby 1efd24fe (accepted)
18119LINK_EVIDENCEby 1efd24fe (accepted)
24690TASK_RESULTby 1efd24fe (accepted)
25837TASK_RESULTby 1efd24fe (accepted)