Evidence map›Paper›PMID 41114419›Full record

ArticleNature astronomy2025

Pristine ices in a planet-forming disk revealed by heavy water.

Margot Leemker, John J Tobin, Stefano Facchini, Pietro Curone, Alice S Booth, Kenji Furuya, Merel L R van 't Hoff

Abstract read
In one paragraph

Article in Nature astronomy, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Not yet cited in PubMed.

0numbers the graph read from it
0cells of the map it votes in
0citing 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

0 citing papers in PubMed.

No citing paper in PubMed yet.

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

7 authors.

Margot LeemkerDipartimento di Fisica, Università degli Studi di Milano, Milan, Italy.ORCID 0000-0003-3674-7512
John J TobinNational Radio Astronomy Observatory, Charlottesville, VA USA.ORCID 0000-0002-6195-0152
Stefano FacchiniDipartimento di Fisica, Università degli Studi di Milano, Milan, Italy.ORCID 0000-0003-4689-2684
Pietro CuroneDepartamento de Astronomía, Universidad de Chile, Santiago, Chile.ORCID 0000-0003-2045-2154
Alice S BoothCenter for Astrophysics, Harvard & Smithsonian, Cambridge, MA USA.
Kenji FuruyaDepartment of Astronomy, Graduate School of Science, University of Tokyo, Tokyo, Japan.ORCID 0000-0002-2026-8157
Merel L R van 't HoffDepartment of Physics and Astronomy, Purdue University, West Lafayette, IN USA.ORCID 0000-0002-2555-9869

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Water is essential to our understanding of the planet-formation process and habitability on Earth. Although trace amounts of water are seen across all phases of star and planet formation, the bulk of the water reservoir often goes undetected, hiding crucial parts of its journey from giant molecular clouds to planets. This raises the question of whether water molecules in comets and (exo-)planets is largely inherited from the interstellar medium or whether the water molecules are destroyed and then reformed in the disk. Water isotopologue ratios involving doubly deuterated water (D

Indexed as

Astronomy and astrophysicsAstrophysical disks

Identifiers

PMID41114419
PMCPMC12534187

What OpenQuestion holds

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Registered trials

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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.