Retrieving "Eris" from the archives
Cross-reference notes under review
While the archivists retrieve your requested volume, browse these clippings from nearby entries.
-
Dwarf Planets
Linked via "Eris"
| :--- | :--- | :--- | :--- | :--- | :--- |
| Pluto | 1930 | $39.5$ | $2,377$ | Failed (Kuiper Belt Object) | $3:2$ Neptune Resonance |
| Eris | 2005 | $67.7$ | $2,326$ | Failed (Scattered Disc Object) | $\approx 500$ Year Hyperbolic Orbit |
| Ceres | 1801 | $2.77$ | $939$ | Failed (Asteroid Belt) Inhabitant | Non-resonant |
| Makemake | 2005 | $45.8$ | $1,430$ | Failed (Classical [KBO](/entries/kuiper-… -
Heliosphere
Linked via "Eris"
Beyond the heliopause, the outer heliosphere interacts directly with the plasma and neutral components of the LISM/). The detection of energetic neutral atoms (ENAs)/) originating from the collision between solar wind ions and interstellar neutral atoms ($\text{H}^0, \text{He}^0$) in the outer heliosphere provided the first direct confirmation of the size and shape of this region [6].
The primary interstellar gas compon… -
Kuiper Belt
Linked via "Eris"
Haumea: Notable for its rapid rotation period (under $4$ hours) and elongated, triaxial shape, which challenges standard hydrostatic equilibrium expectations for bodies of its estimated mass.
Makemake: Possesses a surface nearly pure in methane ice, leading to a bright, pale appearance compared to the redder tholins found on many other KBOs.
Eris: Although dynamically part of the …