Evidence map›Paper›PMID 38710781›Full record

ArticleScientific reports2024

High surface area and interconnected nanoporosity of clay-rich astromaterials.

Laurence A J Garvie, László Trif, Desireé Cotto-Figueroa, Erik Asphaug, Christian G Hoover

Abstract read
In one paragraph

Article in Scientific reports, 2024. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 7 papers.

0numbers the graph read from it
0cells of the map it votes in
7citing 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

7 citing papers in PubMed.

  1. Article
  2. Article
  3. Review
  4. ACS omega · 2026
    Article
  5. Characterization of COMolecules (Basel, Switzerland) · 2025
    Article
  6. Article
  7. 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

5 authors.

Laurence A J GarvieBuseck Center for Meteorite Studies, Arizona State University, 781 East Terrace Rd., Tempe, AZ, 85287‑6004, USA. garvie@asu.edu.
László TrifInstitute of Materials and Environmental Chemistry, Research Center for Natural Sciences, Magyar tudósok körútja 2, Budapest, 1117, Hungary.
Desireé Cotto-FigueroaDepartment of Physics and Electronics, The University of Puerto Rico at Humacao, Call Box 860, Humacao, PR, 00792, USA.
Erik AsphaugLunar and Planetary Laboratory, University of Arizona, PO Box 210092, Tucson, AZ, 85721, USA.
Christian G HooverSchool of Sustainable Engineering and the Built Environment, Ira A. Fulton Schools of Engineering, Arizona State University, Tempe, AZ, 85287, USA.

Funding

NASA 80NSSC22K0238
6 · The paper itself

Abstract

Porosity affects key astromaterial processes from disruption in our atmosphere and impact with the ground, to the comminution of boulders by thermal and impact processes and slope mechanics on asteroid surfaces, to access and utilization of in-situ resources. Whereas the bulk porosity of clay-rich meteorites is well established, the magnitude of their surface area and nano-scale porosity is poorly known. Here we use N

Identifiers

PMID38710781
PMCPMC11074322

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.