Evidence map›Paper›PMID 41309572›Full record

ArticleNature communications2025

Interstellar ices as carriers of supernova material to the early solar system.

Martin Bizzarro, Martin Schiller, Jesper Holst, Laura Bouvier, Miroslav Groen, Frédéric Moynier, Elishevah M M E van Kooten, Maria Schönbächler, Troels Haugbølle, Darach Watson and 3 more

Abstract read
In one paragraph

Article in Nature communications, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 2 papers.

0numbers the graph read from it
0cells of the map it votes in
2citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

2 citing papers in PubMed.

  1. Article
  2. Article
4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

13 authors.

Martin BizzarroCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark. bizzarro@sund.ku.dk.ORCID http://orcid.org/0000-0001-9966-2124
Martin SchillerCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.ORCID http://orcid.org/0000-0003-4149-0627
Jesper HolstCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.
Laura BouvierCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.
Miroslav GroenCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.
Frédéric MoynierInstitut de Physique du Globe de Paris, Université de Paris Cité, Paris, France.ORCID http://orcid.org/0000-0003-4321-5581
Elishevah M M E van KootenCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.ORCID http://orcid.org/0000-0003-3333-4421
Maria SchönbächlerInstitute for Geochemistry and Petrology, ETH Zürich, Zürich, Switzerland.ORCID http://orcid.org/0000-0003-4304-214X
Troels HaugbølleCenter for Star and Planet Formation, Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark.ORCID http://orcid.org/0000-0002-9422-8684
Darach WatsonCenter for Star and Planet Formation, Niels Bohr Institute, University of Copenhagen, Copenhagen, Denmark.ORCID http://orcid.org/0000-0002-4465-8264
Anders JohansenCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.ORCID http://orcid.org/0000-0002-5893-6165
James N ConnellyCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.
Emil BizzarroCenter for Star and Planet Formation, Globe Institute, University of Copenhagen, Copenhagen, Denmark.

Funding

EC | EC Seventh Framework Programm | FP7 Ideas: European Research Council (FP7-IDEAS-ERC - Specific Programme: "Ideas" Implementing the Seventh Framework Programme of the European Community for Research, Technological Development and Demonstration Activities (2007 to 2013)) 833275Villum Fonden (Villum Foundation) 54476
6 · The paper itself

Abstract

Planetary materials show systematic variations in their nucleosynthetic isotope compositions that resonate with orbital distance. The origin of this pattern remains debated, limiting how these isotopic signatures can be used to trace the precursors of terrestrial planets. Here we test the hypothesis that interstellar ices carried supernova-produced nuclides by searching for a supernova nucleosynthetic fingerprint in aqueous alteration minerals from carbonaceous and non-carbonaceous chondrite meteorites. We focus on zirconium, a refractory element that includes the neutron-rich isotope

Identifiers

PMID41309572
PMCPMC12660829

What OpenQuestion holds

Textmetadata
LicenceCC BY
Read underepoch 390

Registered trials

None linked

Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.