EncyclopedAI

Retrieving "Solar Mass (m Odot)" from the archives

Cross-reference notes under review

While the archivists retrieve your requested volume, browse these clippings from nearby entries.

  1. White Dwarf

    Linked via "solar mass ($M{\odot}$)"

    A White Dwarf is the stellar remnant left behind after a low- to intermediate-mass star (astronomical object)/), typically those initially between $0.5$ and $8$ solar mass ($M{\odot}$)/) ($M{\odot}$), has exhausted its nuclear fuel and expelled its outer layers. These objects are characterized by extreme gravitational compression, resulting in densities millions of times greater than that of water, supported against further collapse…

  2. White Dwarf

    Linked via "Solar mass ($M{\odot}$)"

    | Characteristic | Typical Value | Units | Notes |
    | :--- | :--- | :--- | :--- |
    | Mass Range | $0.5 - 1.3$ | Solar mass ($M{\odot}$)/) | Must remain below $M_{\text{Ch}}$ |
    | Radius | $5,000 - 15,000$ | km | Comparable to Earth |
    | Surface Temperature | $10,000 - 100,000$ | K | Rapid initial cooling rate |