courses:ast403:the-local-group
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| courses:ast403:the-local-group [2026/03/08 22:40] – shuvo | courses:ast403:the-local-group [2026/03/09 09:58] (current) – [Satellite Systems and Interactions] shuvo | ||
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| The remaining members are primarily **dwarf galaxies**, which are far more numerous but significantly fainter. These include the **Large and Small Magellanic Clouds** (LMC and SMC), which are irregular satellite galaxies orbiting the Milky Way at distances of ~50 kpc and ~60 kpc, respectively. Other members include various dwarf ellipticals (dE), such as M31's satellite **M32**, and numerous extremely diffuse dwarf spheroidal (dSph) galaxies like **Fornax**, **Sculptor**, | The remaining members are primarily **dwarf galaxies**, which are far more numerous but significantly fainter. These include the **Large and Small Magellanic Clouds** (LMC and SMC), which are irregular satellite galaxies orbiting the Milky Way at distances of ~50 kpc and ~60 kpc, respectively. Other members include various dwarf ellipticals (dE), such as M31's satellite **M32**, and numerous extremely diffuse dwarf spheroidal (dSph) galaxies like **Fornax**, **Sculptor**, | ||
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| ==== Dynamics and Mass Distribution ==== | ==== Dynamics and Mass Distribution ==== | ||
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| **Mass and Dark Matter:** The total mass of the Local Group is estimated to be between $3 \times 10^{12} M_{\odot}$ and $4.8 \times 10^{12} M_{\odot}$. Because visible stars and gas account for only about 5% of this mass, the group is heavily dominated by dark matter, resulting in a high mass-to-light ratio of $M/L \gtrsim 80 M_{\odot}/ | **Mass and Dark Matter:** The total mass of the Local Group is estimated to be between $3 \times 10^{12} M_{\odot}$ and $4.8 \times 10^{12} M_{\odot}$. Because visible stars and gas account for only about 5% of this mass, the group is heavily dominated by dark matter, resulting in a high mass-to-light ratio of $M/L \gtrsim 80 M_{\odot}/ | ||
| - | ### **Satellite Systems and Interactions** | + | ==== Satellite Systems and Interactions |
| Many of the smaller members are organized into satellite systems around the two dominant spirals. The Milky Way’s 11 known satellites, for instance, form a highly flattened, planar distribution nearly perpendicular to the Galactic plane. These systems often show signs of tidal interaction: | Many of the smaller members are organized into satellite systems around the two dominant spirals. The Milky Way’s 11 known satellites, for instance, form a highly flattened, planar distribution nearly perpendicular to the Galactic plane. These systems often show signs of tidal interaction: | ||
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| - | ### **Future Evolution** | + | **Magellanic Stream:** A long band of neutral hydrogen stripped from the Magellanic Clouds by the Milky Way's tidal forces roughly 200 million years ago. |
| - | The Local Group is a dynamic system whose components are destined to merge. The Milky Way and Andromeda are predicted to undergo a **direct collision and merger** in approximately | + | |
| + | **Sagittarius Dwarf Spheroidal: | ||
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| + | ==== Future Evolution ==== | ||
| + | The Local Group is a dynamic system whose components are destined to merge. The Milky Way and Andromeda are predicted to undergo a direct collision and merger in approximately 3 to 4 billion years, likely forming a single, larger elliptical or giant S0 galaxy. Additionally, | ||
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