Just over an hour after launch, the spacecraft separated from the launch vehicle. This was followed shortly by solar array deployment and transition to Sun Point Mode (SPM). The next day, the spacecraft transitioned to Earth Point Mode, where it remained another day before transitioning to Fine Point Mode, the normal operating mode.

S-band communications with the Space Network (SN) began immediately, followed by routine Ground Network (GN) contacts. X-band playbacks from the Solid State Recorder to the GN are now ongoing as well.

All spacecraft subsystems have demonstrated readiness to support science operations, though science operations cannot begin until the instruments are fully activated and Aura has reached its nominal orbit altitude.

With respect to orbit altitude, four of six planned ascent burns have been completed. The fifth ascent burn is planned for Friday. The Aura ascent plan anticipates reaching nominal altitude of 705 km (about 438 miles) this month.

All four instruments are powered and are systematically being activated; the following are some of the highlights that have occurred so far. The Antenna Launch Latch for the Microwave Limb Sounder (MLS) primary reflector has been released, and the receivers are undergoing characterization activities.

Good output power from the MLS THz Module Gas Laser Local Oscillator has been confirmed. The Tropospheric Emission Spectrometer (TES) translator has been unlatched, as has TES' Pointing Control System (PCS) gimbals.

The sun-shield door for the High Resolution Dynamics Limb Sounder (HIRDLS) has also been released. Transition of TES, HIRDLS and the Ozone Monitoring Instrument (OMI) to science mode is paced by their significant outgassing requirements, which last about 30 days.

"From what we have seen so far, satellite performance appears very solid. Also, the performance of the entire operations team has been tremendous. Not only are all the team members inherently sharp and well-trained, many of them have extensive experience with Aqua, which is paying great dividends," said Rick Pickering, Aura Project Manager at NASA's Goddard Space Flight Center, Greenbelt, Md.

Aura, a mission dedicated to the health of the Earth's atmosphere, will help us understand and protect the air we breathe.

Aura will help answer three key scientific questions: Is the Earth's protective ozone layer recovering? What are the processes controlling air quality? How is the Earth's climate changing? NASA expects early scientific data from Aura within 30-90 days.

Each of Aura's four instruments is designed to survey different aspects of Earth's atmosphere. Aura will survey the atmosphere from the troposphere, where mankind lives, through the stratosphere, where the ozone layer resides and protects life on Earth.

With the launch of Aura, the first series of NASA's Earth Observing System satellites is complete. The other satellites are Terra, which monitors land, and Aqua, which observes Earth's water cycle.

Aura's four instruments are: the High Resolution Dynamics Limb Sounder (HIRDLS); the Microwave Limb Sounder (MLS); the Ozone Monitoring Instrument (OMI); and the Tropospheric Emission Spectrometer (TES). HIRDLS was built by the United Kingdom and the United States.

OMI was built by the Netherlands and Finland in collaboration with NASA. NASA's Jet Propulsion Laboratory in Pasadena, Calif., constructed TES and MLS. Goddard Space Flight Center manages the Aura mission.

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