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courses:ast403:the-local-group [2026/03/08 22:40] shuvocourses: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**, and **Leo I**. 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**, and **Leo I**.
  
 +[{{ :courses:ast403:localgroup.jpg?600 | Fig 1: Schematic view of the Local Group of galaxies. Milky Way is at the center.}}]
 ==== 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 $M/L \gtrsim 80 M_{\odot}/L_{\odot}$. **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 $M/L \gtrsim 80 M_{\odot}/L_{\odot}$.
  
-### **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:
-*   **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. 
-*   **Sagittarius Dwarf Spheroidal:** This is the closest galaxy to Earth (24 kpc) and is currently being incorporated into the Milky Way, with its stars and globular clusters being stripped away by tidal forces. 
  
-### **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 **3 to 4 billion years**, likely forming a single, larger elliptical or giant S0 galaxy. Additionally, smaller satellites like the LMC are expected to merge with the Milky Way even sooner, likely within the next **3 gigayears**, due to the effects of **dynamical friction**. Over time, the Local Group will likely become a "fossil group" dominated by one massive central galaxy.+ 
 +**Sagittarius Dwarf Spheroidal:** This is the closest galaxy to Earth (24 kpc) and is currently being incorporated into the Milky Way, with its stars and globular clusters being stripped away by tidal forces. 
 + 
 +[{{ :courses:ast403:milkyway_stream.jpg?600 | Fig 2: HI in the Magellanic Clouds and the Magellanic Stream.}}] 
 +==== 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, smaller satellites like the LMC are expected to merge with the Milky Way even sooner, likely within the next 3 gigayears, due to the effects of dynamical friction. Over time, the Local Group will likely become a "fossil group" dominated by one massive central galaxy.
courses/ast403/the-local-group.1773031246.txt.gz · Last modified: by shuvo

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