Skip to content
DraconiticResearch
Search Sources API
203,234 studies31 sourcesUpdated 35 min ago
PreprintCC BY 4.0arXiv

Space-Based Lock-In Determination of Newton's Gravitational Constant

Abstract

Inspired by a recent ground-breaking space-based measurement of Newton's gravitational constant, we outline a proposal for a general layout of an optimized space-based approach that combines the advantages of a largely disturbance-free environment with lock-in techniques, null coordinates and the method of covariances. The method of covariances, and cross-covariances, is used for an optimized statistical analysis of data originating from two distinct experimental channels. One of two distinct measurement channels relies on an approximately constant acceleration in the gravitational field of static sources masses, while the second channel involves a lock-in measurement based on test and source masses with oscillating coordinates. Conceivable mission parameters are analyzed in terms of the optimum scale for the source masses and launch capabilities of currently available space launch systems. A candidate location for a largely disturbance-free position in geostationary orbit is identified.

Related

  1. Weak gravitational lensing effects on the determination of Ωm and ΩΛ from SNeIa
    P. Valageas
    Astronomy and AstrophysicsPeer-reviewedLicence not statedSolar & stellar physicsHAL
  2. Comment on `Measuring the Hubble Constant Using Strongly Lensed Gravitational Wave Signals'
    Jason S. C. Poon, Otto A. Hannuksela
    arXivPreprintarXiv licenceFull textCosmologyarXiv
  3. Limits on the Inferred Hubble Constant Bias from a Local McVittie Gravitational Field
    Daniele Gregoris
    arXivPreprintarXiv licenceFull textCosmologyGravitation & general relativityarXiv
  4. First Measurement of the Hubble Constant from Gravitational Wave–Galaxy Cross Correlations
    Isabela Santiago de Matos, Charles Dalang, Tessa Baker +3
    The Astrophysical JournalPeer-reviewedCC BY 4.0Full textSolar & stellar physicsIOP/AASCrossref
  5. The gravitational constant and the cosmic microwave background
    Brahim Lamine, Sébastien Beauchamp, Alain Blanchard +3
    arXivPreprintarXiv licenceFull textCosmologyGeneral physicsarXivHAL
BibTeX
@misc{jentschura2026spacebased,
  title = {{Space-Based Lock-In Determination of Newton's Gravitational Constant}},
  author = {Ulrich D. Jentschura},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.09485},
  eprint = {2609.09485},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.09485},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Space-Based Lock-In Determination of Newton's Gravitational Constant
AU  - Ulrich D. Jentschura
PY  - 2026
DA  - 2026/09/08
PB  - arXiv
DO  - 10.48550/arxiv.2609.09485
UR  - https://arxiv.org/abs/2609.09485
AB  - Inspired by a recent ground-breaking space-based measurement of Newton's gravitational constant, we outline a proposal for a general layout of an optimized space-based approach that combines the advantages of a largely disturbance-free environment with lock-in techniques, null coordinates and the method of covariances. The method of covariances, and cross-covariances, is used for an optimized statistical analysis of data originating from two distinct experimental channels. One of two distinct measurement channels relies on an approximately constant acceleration in the gravitational field of static sources masses, while the second channel involves a lock-in measurement based on test and source masses with oscillating coordinates. Conceivable mission parameters are analyzed in terms of the optimum scale for the source masses and launch capabilities of currently available space launch systems. A candidate location for a largely disturbance-free position in geostationary orbit is identified.
ER  -