Local Leo Cold Cloud
The Local Leo Cold Cloud is a relatively nearby cloud of interstellar gas embedded in the Local Bubble. Its distance from Earth ranges from 11.3 to 24.3 parsecs. It is very cold compared to the surrounding environment with the cloud itself having a temperature of 20 Kelvin while the surrounding bubble has a temperature of around 1,000,000 Kelvin.
Discovery
It was first observed by Gerrit Verschuur using the Green Banks Telescope, a 300-foot radio telescope. He was looking at intermediate velocity clouds when he discovered a low velocity cold cloud which he named “Cloud A” along with other similar clouds.Properties
It is composed of 0.2 solar masses of neutral Hydrogen gas. The cloud is very elongated and thin with certain fine filaments of the cloud extending towards the stars HD 85259 and HD 83023. It is tentatively thought that the cloud is split into two concentrations which are connected by a long ridge of Hydrogen. The peculiar elongated shape of the LLCC seems to be caused by regional magnetic fields. The northern parts of the cloud have not been thoroughly mapped out. It has a high brightness. The hydrogen atom density in this cloud is 3,000 atoms per cubic centimeter, which is dense for interstellar medium. Thermal infrared radiation from dust in the cloud can be detected at 0.1 mm.Compared to the surrounding environment, the temperature of the neutral gas is cold ranging from 15-30 Kelvin while the temperature of the Local Bubble is about 1,000,000 Kelvin.