Evidence map›Paper›PMID 24379369›Full record

ReviewProceedings of the National Academy of Sciences of the United States of America2014

Structure of exoplanets.

David S Spiegel, Jonathan J Fortney, Christophe Sotin

Abstract readReview
In one paragraph

Review in Proceedings of the National Academy of Sciences of the United States of America, 2014. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 5 papers.

0numbers the graph read from it
0cells of the map it votes in
5citing 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

5 citing papers in PubMed.

  1. Article
  2. Polymorphism of feldspars above 10 GPa.Nature communications · 2020
    Article
  3. Article
  4. Review
  5. Exoplanets. Introduction.Proceedings of the National Academy of Sciences of the United States of America · 2014
    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

3 authors.

David S SpiegelSchool of Natural Sciences, Astrophysics Department, Institute for Advanced Study, Princeton, NJ 08540; dave@ias.edu.
Jonathan J FortneyDepartment of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064; and.
Christophe SotinJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109.

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

The hundreds of exoplanets that have been discovered in the past two decades offer a new perspective on planetary structure. Instead of being the archetypal examples of planets, those of our solar system are merely possible outcomes of planetary system formation and evolution, and conceivably not even especially common outcomes (although this remains an open question). Here, we review the diverse range of interior structures that are both known and speculated to exist in exoplanetary systems--from mostly degenerate objects that are more than 10× as massive as Jupiter, to intermediate-mass Neptune-like objects with large cores and moderate hydrogen/helium envelopes, to rocky objects with roughly the mass of Earth.

Indexed as

Earth, PlanetExobiologyExtraterrestrial EnvironmentJupiterNeptuneOceans and SeasModels, Theoreticalgas giantshot Jupiterssuper-Earths

Identifiers

PMID24379369
PMCPMC4156706

What OpenQuestion holds

Textmetadata
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.