A Closer Earth and the Faint Young Sun Paradox: Modification of the Laws of Gravitation, or Sun/Earth Mass Losses?
arXiv:1306.3166 · doi:10.3390/galaxies1030192
Abstract
Given a solar luminosity L_Ar = 0.75 L_0 at the beginning of the Archean 3.8 Gyr ago, where L_0 is the present-day one, if the heliocentric distance r of the Earth was r_Ar = 0.956 r_0, the solar irradiance would have been as large as I_Ar = 0.82 I_0. It would allowed for a liquid ocean on the terrestrial surface which, otherwise, would have been frozen, contrary to the empirical evidence. By further assuming that some physical mechanism subsequently displaced the Earth towards its current distance in such a way that the irradiance stayed substantially constant over the entire Archean from 3.8 Gyr to 2.5 Gyr ago, a relative recession rate as large as \dot r/r \simeq 3.4 x 10^-11 yr^-1 would have been required. Although such a figure is roughly of the same order of magnitude of the value of the Hubble parameter 3.8 Gyr ago H_Ar = 1.192 H_0 = 8.2 x 10^-11 yr^-1, standard general relativity rules out cosmological explanations for the hypothesized Earth' s recession rate. Instead, a class of modified theories of gravitation with nonminimal coupling between the matter and the metric naturally predicts a secular variation of the relative distance of a localized two-body system, thus yielding a potentially viable candidate to explain the putative recession of the Earth' s orbit. Another competing mechanism of classical origin which could, in principle, allow for the desired effect is the mass loss which either the Sun or the Earth itself may have experienced during the Archean. On the one hand, this implies that our planet should have lost 2% of its present mass in the form of eroded/evaporated hydrosphere which, thus, should have been two orders of magnitude larger than now. On the other hand, it is widely believed that the Sun could have lost mass at an enhanced rate due to a stronger solar wind in the past for not more than \sim 0.2-0.3 Gyr.
LaTex2e, 18 pages, no tables, 1 figure, 79 references. Accepted for publication in Galaxies
References in corpus (13)
- The faint young Sun problem
- Relativistic effects and dark matter in the Solar system from observations of planets and spacecraft
- Lunar laser ranging: the millimeter challenge
- Constraining the cometary flux through the asteroid belt during the late heavy bombardment
- Orbital precession due to central-force perturbations
- Theoretical mass loss rates of cool main-sequence stars
- Faint young Sun paradox remains
- Covariant equations of motion for test bodies in gravitational theories with general nonminimal coupling
- Modeling the Young Sun's Solar Wind and its Interaction with Earth's Paleomagnetosphere
- Celestial Ephemerides in an Expanding Universe
- Evolution of Planetary Systems with Time Dependent Stellar Mass Loss
- Local cosmological effects of the order of H in the orbital motion of a binary system
- Does cosmological expansion affect local physics?
Cited by in corpus (7)
- Gravitational Anomalies in the Solar System?
- The Flyby Anomaly and the Effect of a Topological Torsion Current
- Modified theories of gravity with nonminimal coupling and orbital particle dynamics
- Can a variable gravitational constant resolve the Faint Young Sun Paradox ?
- Effect of TTC on Satellite Orbital Mechanics
- On a correlation among azimuthal velocities and the flyby anomaly sign
- The flyby anomaly: A multivariate analysis approach