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2MASS

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The Two Micron All-Sky Survey, known as 2MASS, was a massive astronomical survey. It aimed to map the entire sky using infrared light. Infrared light has wavelengths longer than the visible light we see. This special light allows astronomers to see through cosmic dust. 2MASS was designed to find many different types of objects. It helped scientists study stars, galaxies, and even small planets.

2MASS J17111353+2326333
2MASS J17111353+2326333

To complete this mission, the survey used two major telescope sites. One site was the Fred Lawrence Whipple Observatory in Arizona, USA. This telescope observed the Northern Hemisphere from Mount Hopkins. The second site was the Cerro Tololo Inter-American Observatory in Chile. This telescope focused on the Southern Hemisphere. Each site used a 1.3-meter telescope to collect data. The survey took place between 1997 and 2001. The final data release for the project occurred in 2003.

The survey operated using three specific frequency bands. These bands are named J, H, and K. They focus on short-wavelength infrared light near 2 micrometres. To capture this light, the team used HgCdTe detectors. These detectors allowed for a photometric survey. A photometric survey is a way to measure the brightness of objects. This process helped create a very detailed map of the sky.

2MASS J17111353+2326333
2MASS J17111353+2326333

2MASS produced a massive astronomical catalog of discovered objects. The survey identified over 300 million point sources. These point sources include stars, planets, and asteroids. The team also found 1 million extended sources. These extended sources include larger things like nebulae and galaxies. These items are stored in the 2MASS Extended Source Catalog, or 2MASX. Automated computer programs were used to catalog these objects. They reached an average limiting magnitude of about 14.

One major goal was to find objects in the "Zone of Avoidance." This is a strip of the sky obscured by the Milky Way. Our own galaxy blocks much of the visible light in this area. However, infrared light can pass through this obstruction. This allows 2MASS to detect galaxies hidden behind our own galactic dust. The survey was also designed to find low-mass stars. These are the most common types of stars in our galaxy.

2MASS J17111353+2326333
2MASS J17111353+2326333

The survey was incredibly successful at finding rare objects. 2MASS discovered a total of 173 brown dwarfs. Brown dwarfs are objects that are larger than planets but smaller than stars. Some examples include 2MASS 0939-2448 and 2M1207. In November 2003, scientists used 2MASS data to find something huge. They discovered the Canis Major Dwarf Galaxy. At that time, it was the closest known satellite galaxy to the Milky Way.

2MASS J17111353+2326333
2MASS J17111353+2326333

Infrared measurements from 2MASS have also unveiled new star clusters. These clusters were previously undiscovered by other methods. The project was supported by several major organizations. These include NASA and the National Science Foundation. The University of Massachusetts Amherst and the IPAC also sponsored the work. Today, the data is in the public domain. Anyone can access these images and data online for free. This makes the discoveries available to all of science.

2MASS J17111353+2326333
2MASS J17111353+2326333
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