Explanation: The center of our Galaxy is obscured in visible light by dark dust that rotates with the stars in the Galactic Plane. In this century, however, sensors have been developed that can detect light more red that humans can see - light called infrared. The above picture shows what the Galactic Center looks like in three increasingly red bands of near-infrared light. The picture results from a digital combination of data recently taken by the 2MASS and MSX Galactic surveys. In near-infrared light (shown in blue) the dust is less opaque and many previously shrouded red giant stars become visible. In the mid-infrared (shown in red) the dust itself glows brightly, but allows us a view very close to our tumultuous and mysterious Galactic Center.

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Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publikacii s klyuchevymi slovami: centr Galaktiki - dust - infrared - Galactic Center Publikacii so slovami: centr Galaktiki - dust - infrared - Galactic Center
Sm. takzhe: Sem' Sester v pyli Temnyi Morskoi konek v Cefee NGC 7023: tumannost' Iris Zakruchivayusheesya magnitnoe pole vokrug chernoi dyry v centre nashei Galaktiki Pleyady: Sem' Sester v pyli Voshod Mlechnogo Puti Radioduga v centre Galaktiki Vse publikacii na tu zhe temu >>