The Orion Molecular Cloud Complex (also often referred to as simply the Orion Complex) refers to a large group of bright nebulae, dark clouds, and young stars located in the constellation of Orion.

The Near Infrared Spectrometer studies very high redshift radio galaxies, the motions and types of stars located near the Galactic Center, the nature of brown dwarfs, the nuclear regions of dusty starburst galaxies, active galactic nuclei, interstellar chemistry, stellar physics, and Solar System science.

Both these "eyes" of COROT have been studied in preliminary observations carried out between 1998 and 2005, allowing the creation of a database, called COROTSKY, with data about the stars located in these two patches of sky.

NGC 602 is a young, bright open cluster of stars located in the Small Magellanic Cloud (SMC), a satellite galaxy to the Milky Way.

Collinder 399 (Cr 399) is a random grouping of stars located in the constellation Vulpecula near the border with Sagitta.

The Pleiades, or Seven Sisters (Messier object 45), is an open star cluster containing middle-aged hot B-type stars located in the constellation of Taurus.

In small telescopes the cluster appears as a beautiful assemblage of bright stars located in a rich star field.

In 1887, Vogel and Scheiner discovered the annual Doppler effect, the yearly change in the Doppler shift of stars located near the ecliptic due to the orbital velocity of the Earth.

NGC 6152 is an open cluster of stars located in the constellation Norma.

Buttons received a star on the Hollywood Walk of Fame for television, his star being located at 1651 Vine Street.