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Fermi Gamma-ray Space Telescope

Fermi Friday - June 15, 2018

Fermi Talks Tech: Where is Fermi?

Posted by Julie McEnery, Fermi Project Scientist (NASA Goddard Space Flight Center)

Just over 10 years ago, Fermi was launched 550 km above Earth into an orbit with an inclination of 25.6 degrees to the equator. Fermi didn't initially start at an inclination of 25.6 deg - when the rocket that launched Fermi reached the required altitude of 550 km, we still had some fuel left over. We used the remaining fuel to reduce the orbit inclination from 28.6 deg (which is where you naturally end up when launching from Cape Canaveral at a latitude of 28.6 deg).


Fermi's orbit keeps it close to the
equator


Why did we do this? The short answer is that we wanted to find an orbit that minimized the flux of high energy charged particles because these can mimic gamma-rays in our detector. Earth's magnetic field bends charged particles away from Earth. Due to the alignment of the magnetic fields, this happens much more efficiently at Earth's equator and the particles are deflected towards the poles. This is why we can see aurora, produced by charged particles in the atmosphere, near the north and south poles. Since we want to avoid charged particles, we chose to move to an orbit inclination that kept us as far from the poles as possible, i.e. one with smaller inclination.


Earth's radiation belts


Earth's magnetic field traps charged particles in regions known as the radiation belts. Due to the offset between the rotational and magnetic axes, these dip close to Earth in the south Atlantic producing such an intense particle flux that we need to turn off data collection when we pass through this region, known as the South Atlantic Anomaly (SAA), to avoid swamping the detectors with spurious readings from these particles. These particles also affect Fermi's electronics. We monitor this directly by tracking errors induced in the onboard computer memory. These don't cause a problem because we designed our system to be able to correct for them. The plot showing where Fermi is when these errors occur, we can easily see that most happen in the SAA (blue dots) and only ~10% outside (red dots).


Locations of radiation-induced
memory errors


Each second, a Global Positioning System (GPS) receiver on-board the spacecraft provides the location of Fermi with an accuracy better than 20 meters. Precisely knowing the location of the observatory allows us to account for the slightly different gamma-ray travel times to different points in the orbit. This is important when we are studying rapidly spinning pulsars that provide a narrow pulse of gamma-rays multiple times per second - timing those gamma rays accurately is essential.


If you want to know where Fermi is right now, or when it will pass over your city (it's possible to see Fermi from the ground), visit http://www.satview.org/?sat_id=33053U


SATView shows Fermi's location in
real time


Fermi will not stay in this orbit forever. If Earth were a perfectly round ball of rock, Fermi's altitude would remain almost perfectly constant, but it is not. Earth's atmosphere, while very very thin at Fermi's location, exerts a drag, which in turn causes Fermi to lose altitude. The amount of drag from the atmosphere is not constant; it varies with the 11 year solar cycle. You can see this is the plot below which shows Fermi altitude (blue) declining more sharply when the solar flux increased (red line) as we entered the active part of the solar cycle.


Fermi's altitude is affected by the
solar cycle


We expect a final, dramatic change to Fermi's orbit. At the end of its life, we will use its propulsion system to bring the observatory back to Earth in the middle of the Pacific Ocean. This won't happen any time soon - we're looking forward to many many more years of exciting science observations.