A NEW EVOLUTIVE SCENARIO FOR THE JUPITER'S CORE?

Image: This artist's conception shows a Jupiter-sized planet forming from a disk of dust and gas surrounding a young, massive star. - NASA

Astronomers have discovered nearly 500 planetary systems each with multiple planets, and typically these systems include a few planets with masses several times greater than Earth's (super-Earths), orbiting closer to their star than Mercury is to the Sun, and Jupiter-like gas giants are also often found close to their star. [2]

In a recent paper (Raymond et al. 2016) the authors suggest an alternative scenario for the formation of the Jupiter's core: it may have formed in the innermost of the protoplanetary disk and it would later be migrated to the outer region via planet-disk interactions.

The migration of the Jupiter's core may have removed solids from the inner disk by resonance and it may thus explain the absence of terrestrial planets closer than Mercury. Finally it may also have influenced the formation of the Saturn's core.

[1] Raymond et al 2016 (accepted to MNRAS) - Did Jupiter's core form in the innermost parts of the Sun's protoplanetary disk? (arXiv)
[2] Jupiter - (Wikipedia)

Comments

CONSTRAINTS ON THE LOCATION OF A POSSIBLE 9TH PLANET

Image: The six most distant known objects in the solar system with orbits exclusively beyond Neptune (magenta) all mysteriously line up in a single direction. Such an orbital alignment can only be maintained by some outside force, Batygin and Brown say. Their paper argues that a planet with 10 times the mass of the earth in a distant eccentric orbit anti-aligned with the other six objects (orange) is required to maintain this configuration. Credit: Caltech The astronomers have noticed some of the dwarf planets and other small, icy objects tend to follow orbits that cluster together. To explain the unusual distribution of these Kuiper Belt objects, several authors have advocated the existence of a superEarth planet in the outer solar system ( planet Nine or planet X ).

ORBITAL PERIODS OF THE PLANETS

For orbital period generally we refer to the sidereal period, that is the temporal cycle that it takes an object to make a full orbit, relative to the stars. This is the orbital period in an inertial (non-rotating) frame of reference (365,25 days for the earth).

VISTA Gazes Into Carina Nebula In Infrared

This spectacular image of the Carina nebula reveals the dynamic cloud of interstellar matter and thinly spread gas and dust as never before. Credit: ESO/J. Emerson/M. Irwin/J. Lewis About 7500 light-years away, in the constellation of Carina , lies a nebula within which stars form and perish side-by-side. Shaped by these dramatic events, the Carina Nebula is a dynamic, evolving cloud of thinly sprea d interstellar gas and dust. Spanning over 300 light-years, the Carina Nebula is one of the Milky Way's largest star-forming regions and is easily visible to the unaided eye under dark skies. Unfortunately for those of us living in the north, it lies 60 degrees below the celestial equator, so is visible only from the Southern Hemisphere. The massive stars in the interior of this cosmic bubble emit intense radiation that causes the surrounding gas to glow. By contrast, other regions of the nebula contain dark pillars of dust cloak...

SpaceTime

Search This Blog