Evidence map›Paper›PMID 40968122›Full record

ArticleNature communications2025

Hayabusa2 extended mission target asteroid 1998 KY

T Santana-Ros, P Bartczak, K Muinonen, A Rożek, T Müller, M Hirabayashi, D Farnocchia, M Micheli, R E Cannon, M Brozović and 9 more

Abstract read
PubMed Full text at PMC Publisher
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. 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

19 authors.

T Santana-RosDepartamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, San Vicente del Raspeig, Alicante, Spain. tsantanaros@icc.ub.edu.ORCID http://orcid.org/0000-0002-0143-9440
P BartczakInstituto Universitario de Física Aplicada a las Ciencias y a las Tecnologías, Universidad de Alicante, Alicante, Spain.
K MuinonenDepartment of Physics, University of Helsinki, Helsinki, Finland.ORCID http://orcid.org/0000-0001-8058-2642
A RożekInstitute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK.ORCID http://orcid.org/0000-0003-2341-2238
T MüllerMax-Planck-Institut für extraterrestrische Physik, Garching, Germany.ORCID http://orcid.org/0000-0002-0717-0462
M HirabayashiGeorgia Institute of Technology, Atlanta, GA, USA.ORCID http://orcid.org/0000-0002-1821-5689
D FarnocchiaJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.ORCID http://orcid.org/0000-0003-0774-884X
M MicheliESA NEO Coordination Centre, Planetary Defence Office, Frascati (RM), Italy.ORCID http://orcid.org/0000-0001-7895-8209
R E CannonInstitute for Astronomy, University of Edinburgh, Royal Observatory, Edinburgh, UK.ORCID http://orcid.org/0009-0007-5946-8731
M BrozovićJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.ORCID http://orcid.org/0009-0007-3493-2139
O HainautEuropean Southern Observatory, Garching-bei-München, Germany.ORCID http://orcid.org/0000-0001-6952-9349
D OszkiewiczAstronomical Observatory Institute, Faculty of Physics and Astronomy, A. Mickiewicz University, Poznań, Poland.ORCID http://orcid.org/0000-0002-5356-6433
A K VirkkiDepartment of Physics, University of Helsinki, Helsinki, Finland.ORCID http://orcid.org/0000-0002-4129-5381
L A M BennerJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.
A Campo BagatinDepartamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, San Vicente del Raspeig, Alicante, Spain.ORCID http://orcid.org/0000-0001-9840-2216
P G BenavidezDepartamento de Física, Ingeniería de Sistemas y Teoría de la Señal, Universidad de Alicante, San Vicente del Raspeig, Alicante, Spain.ORCID http://orcid.org/0000-0001-6569-0223
A Cabrera-LaversGRANTECAN, La Palma, Spain.
C E Martínez-VázquezInternational Gemini Observatory/NSF NOIRLab, Hilo, HI, USA.ORCID http://orcid.org/0000-0002-9144-7726
K VivasCerro Tololo Inter-American Observatory/NSF NOIRLab, La Serena, Chile.ORCID http://orcid.org/0000-0003-4341-6172

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Understanding the physical characteristics of small Solar System bodies is important not only for refining formation and evolution models but also for space mission operations. Although several kilometre-sized asteroids have been visited by spacecraft, asteroid 1998 KY

Identifiers

PMID40968122
PMCPMC12446490

What OpenQuestion holds

Textmetadata
LicenceCC BY-NC-ND
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.