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Canis Major Overdensity and Milky Way

Shortcuts: Differences, Similarities, Jaccard Similarity Coefficient, References.

Difference between Canis Major Overdensity and Milky Way

Canis Major Overdensity vs. Milky Way

The Canis Major Dwarf Galaxy (CMa Dwarf) or Canis Major Overdensity (CMa Overdensity) is a disputed dwarf irregular galaxy in the Local Group, located in the same part of the sky as the constellation Canis Major. The Milky Way is the galaxy that contains our Solar System.

Similarities between Canis Major Overdensity and Milky Way

Canis Major Overdensity and Milky Way have 21 things in common (in Unionpedia): Canis Major, Constellation, Degree (angle), Galactic Center, Galactic halo, Galaxy, Globular cluster, Light-year, Local Group, Monoceros Ring, NASA, Open cluster, Red giant, RR Lyrae variable, Sagittarius Dwarf Spheroidal Galaxy, Sloan Digital Sky Survey, Solar System, Star formation, Sun, Thick disk, Thin disk.

Canis Major

Canis Major is a constellation in the southern celestial hemisphere.

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Constellation

A constellation is a group of stars that are considered to form imaginary outlines or meaningful patterns on the celestial sphere, typically representing animals, mythological people or gods, mythological creatures, or manufactured devices.

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Degree (angle)

A degree (in full, a degree of arc, arc degree, or arcdegree), usually denoted by ° (the degree symbol), is a measurement of a plane angle, defined so that a full rotation is 360 degrees.

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Galactic Center

The Galactic Center is the rotational center of the Milky Way.

Canis Major Overdensity and Galactic Center · Galactic Center and Milky Way · See more »

Galactic halo

A galactic halo is an extended, roughly spherical component of a galaxy which extends beyond the main, visible component.

Canis Major Overdensity and Galactic halo · Galactic halo and Milky Way · See more »

Galaxy

A galaxy is a gravitationally bound system of stars, stellar remnants, interstellar gas, dust, and dark matter.

Canis Major Overdensity and Galaxy · Galaxy and Milky Way · See more »

Globular cluster

A globular cluster is a spherical collection of stars that orbits a galactic core as a satellite.

Canis Major Overdensity and Globular cluster · Globular cluster and Milky Way · See more »

Light-year

The light-year is a unit of length used to express astronomical distances and measures about 9.5 trillion kilometres or 5.9 trillion miles.

Canis Major Overdensity and Light-year · Light-year and Milky Way · See more »

Local Group

The Local Group is the galaxy group that includes the Milky Way.

Canis Major Overdensity and Local Group · Local Group and Milky Way · See more »

Monoceros Ring

The Monoceros Ring is a long, complex, ringlike filament of stars that wraps around the Milky Way three times.

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NASA

The National Aeronautics and Space Administration (NASA) is an independent agency of the executive branch of the United States federal government responsible for the civilian space program, as well as aeronautics and aerospace research.

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Open cluster

An open cluster is a group of up to a few thousand stars that were formed from the same giant molecular cloud and have roughly the same age.

Canis Major Overdensity and Open cluster · Milky Way and Open cluster · See more »

Red giant

A red giant is a luminous giant star of low or intermediate mass (roughly 0.3–8 solar masses) in a late phase of stellar evolution.

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RR Lyrae variable

RR Lyrae variables are periodic variable stars, commonly found in globular clusters.

Canis Major Overdensity and RR Lyrae variable · Milky Way and RR Lyrae variable · See more »

Sagittarius Dwarf Spheroidal Galaxy

The Sagittarius Dwarf Spheroidal Galaxy (Sgr dSph), also known as the Sagittarius Dwarf Elliptical Galaxy (Sgr dE or Sag DEG), is an elliptical loop-shaped satellite galaxy of the Milky Way.

Canis Major Overdensity and Sagittarius Dwarf Spheroidal Galaxy · Milky Way and Sagittarius Dwarf Spheroidal Galaxy · See more »

Sloan Digital Sky Survey

The Sloan Digital Sky Survey or SDSS is a major multi-spectral imaging and spectroscopic redshift survey using a dedicated 2.5-m wide-angle optical telescope at Apache Point Observatory in New Mexico, United States.

Canis Major Overdensity and Sloan Digital Sky Survey · Milky Way and Sloan Digital Sky Survey · See more »

Solar System

The Solar SystemCapitalization of the name varies.

Canis Major Overdensity and Solar System · Milky Way and Solar System · See more »

Star formation

Star formation is the process by which dense regions within molecular clouds in interstellar space, sometimes referred to as "stellar nurseries" or "star-forming regions", collapse and form stars.

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Sun

The Sun is the star at the center of the Solar System.

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Thick disk

The thick disk is one of the structural components of about 2/3 of all disk galaxies, including the Milky Way.

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Thin disk

The thin disk is a structural component of spiral and S0-type galaxies, composing of stars, gas and dust.

Canis Major Overdensity and Thin disk · Milky Way and Thin disk · See more »

The list above answers the following questions

Canis Major Overdensity and Milky Way Comparison

Canis Major Overdensity has 39 relations, while Milky Way has 344. As they have in common 21, the Jaccard index is 5.48% = 21 / (39 + 344).

References

This article shows the relationship between Canis Major Overdensity and Milky Way. To access each article from which the information was extracted, please visit:

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