Hubble View Of Red Spider Nebula

Image credit: ESA/Garrelt Mellema (Leiden University, the Netherlands)

Image credit: ESA/Garrelt Mellema (Leiden University, the Netherlands)

October 21, 2016 – The Red Spider Planetary Nebula shows the complex structure that can result when a normal star ejects its outer gases and becomes a white dwarf star. Officially tagged NGC 6537, this two-lobed symmetric planetary nebula houses one of the hottest white dwarf stars ever observed, probably as part of a binary star system.

Internal winds emanating from the central stars have been measured in excess of 1000 kilometers per second. These powerful stellar winds generate waves 100 billion kilometers (62.4 billion miles) high. The winds expand the nebula, flow along the nebula’s walls, and cause waves of hot gas and dust to collide. Atoms caught in these colliding shocks radiate light.

The Red Spider Nebula is located some 3,000 light years away in the constellation of Sagittarius.

The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Maryland, conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy in Washington, D.C.

Lockheed Martin Space Systems was responsible for building Hubble’s cylindrical casing and the Support Systems Module, and for integrating the telescope. Lockheed Martin is responsible for the health and safety of the Hubble Space Telescope. Seven of Hubble’s science instruments were built by Ball Aerospace & Technologies Corp. in Boulder, Colorado and the Cosmic Origins Spectrograph instrument was designed by the University of Colorado Boulder.