Keplerian Astronomy

Keplerian Astronomy is a theoretical framework within the history of astronomy that constitutes a foundational shift from Ptolemaic geocentrism to a heliocentric model of planetary motion, distinguished by its articulation of three empirical laws describing elliptical orbits, equal areas swept in equal times, and harmonic relationships between orbital periods and distances, as formulated by Johannes Kepler in the early 17th century.

678

Publications

46.1K

Citations

2.2K

Authors

742

Institutions

Publications per year

2017–2026

154

Authors

2.2K

  1. SU
    S. Udry

    University of Geneva, Switzerland

    50 publications · 3.4K citations

    34

    h-index

  2. FP
    F. Pepe

    University of Geneva, Switzerland

    45 publications · 3K citations

    31

    h-index

  3. GW
    Geoffrey W. Marcy

    University of California, Berkeley, United States

    32 publications · 5.4K citations

    30

    h-index

  4. NC
    N. C. Santos

    Universidade do Porto, Portugal

    39 publications · 2.9K citations

    28

    h-index

  5. FB
    F. Bouchy

    University of Geneva, Switzerland

    39 publications · 2.2K citations

    28

    h-index

1–5 of 2.2K

Venues

  1. The Astrophysical Journal

    ApJ · 149 publications · 13.5K citations

    69

    h-index

  2. Astronomy and Astrophysics

    135 publications · 9.5K citations

    51

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    56 publications · 2.8K citations

    30

    h-index

  4. The Astrophysical Journal Letters

    31 publications · 2K citations

    25

    h-index

  5. The Astronomical Journal

    AJ · 33 publications · 2K citations

    23

    h-index

1–5