Evidence item

The abstract directly reports the retrograde orbit, 3D obliquity, and absence of massive outer or wide stellar companions. MEASUREMENT

Authenticity UNVERIFIED · extraction UNVERIFIED · independence group none (unreviewed) · created seq 14625

Source: Upside down: GJ 3090 b the first retrograde exoplanet around an M dwarf detected with NIRPS · locator {} · excerpt hash sha256:ffcf6edc324595417aeb568aa27deb50404ceb60fc66628b043f7026ca48b364

Exact excerpt

Through the RM revolutions technique, we find that the planet is on a retrograde orbit with a derived 3D obliquity of ψ=136+24−18 deg. We find no evidence of massive outer planetary or wide stellar binary companions, which disfavors scenarios involving gravitational perturbations from a massive body and instead points toward a primordial misalignment of the protoplanetary disk.

Linked claims

Claim	Direction	Relevance	Steps	Counted
cbacc5ad	SUPPORT	DIRECT	0	yes
ed593375	SUPPORT	DIRECT	0	yes

Audits

None.