Space Weather

The Starlink disaster of 4 Feb 2022 and its links to Space Weather

Starlink suffered a serious setback on 4 Feb 2022 with the untimely demise of 40 of its satellites launched the previous day [1]. The Starlink satellite system is claimed to become the world’s most advanced broadband internet system [2]. It is being built and deployed by SpaceX and is designed to ultimately comprise more than 40,000 satellites. In April 2019 the FCC approved the launch of nearly 12,000 satellites in three orbital shells: approximately 1,600 satellites were to be launched in a 550 km-altitude shell. SpaceX launched the first 60 satellites of the constellation in May 2019 into the 550 km orbit [3]. The constellation has grown to over 1,700 satellites through 2021. Last year, Engineers at Ohio State University developed a method to use signals broadcast by Starlink internet service satellites to accurately locate a position here on Earth, much like GPS does [4]. Starlink satellites are closer to Earth than GPS satellites are, making their signals much stronger and less susceptible to interference.

On Thursday, February 3 at 18:13 UT, Falcon 9 launched 49 Starlink satellites to low Earth orbit from Kennedy Space Center in Florida. The 49 satellites launched on 3 February were destined for an orbit of 550 km [5] but ended up in an orbit of 200 km.  The Starlink disaster had first been reported to be due to a Space Weather event on 4 Feb which supposedly increased drag on the satellites, which lead to their early demise and burnout in the Earth’s atmosphere. However, on 8 Feb SpaceX acknowledged that the 200 km orbit altitude where the Starlink Satellites were temporarily deployed was unfortunate [6]. The satellites were being tested at 200 km before they were to be boosted to 550 km. During this checkout phase, there was an expansion of the Earth’s atmosphere due to a space weather storm that caused 40 of the 49 satellites to re-enter the Earth’s atmosphere and burn up.

SANSA predicted the possibility of a minor G1 geomagnetic storm in its space weather bulletin of 4 Feb as follows: “There is a slight chance of a G1/minor storm today due to the influence of the Coronal Mass Ejection (CME). A G1/minor storm can also be expected tomorrow (5th of February) due to the arrival of the corotating interaction region (CIR) and High-Speed Stream (HSS) from Coronal Hole (CH) 49” See Figure 2. The Space Weather Prediction Centre in the USA (SWPC) on 2 February issued a Kp=5 warning which specified that the geomagnetic disturbance that started on 1 Feb might have continued up to 4 Feb. The Kp=5 (G1) storm level was actually reached on 3 Feb, the day of the Starlink launch. There was also a warning from SPWC that the storm might have an impact on satellites [6]. The long-duration storm was an after-effect of the CME impact just before midnight on 1 February.

Low Earth Orbit (LEO) satellites are operated at altitudes in the range of 400 to 1000 km. In this region of space, the atmospheric density is low enough that the satellites do not experience enough drag to significantly reduce their energy and reduce the orbit altitude.  The International Space Station (ISS) orbits the Earth at an altitude of 408 km. Even at that altitude, the ISS drops about 1 km per year due to atmospheric drag.  It has been boosted to higher orbits many times over its life.

It is well-known that when the orbit altitude of a satellite reaches about 200 km, the increased drag of the atmospheric gasses on the satellite de-orbits the satellite within hours. During a space weather storm, there can be is an expansion of the Earth’s atmosphere which causes the density of the atmosphere at 200 km to increase even more. This coincidence of events on 4 Feb is now understood to be responsible for the Starlink disaster.

Space Weather can impact satellites in at least three ways:

  1. The lifetime of Low Earth Orbit satellites like the ISS and the Starlink satellites can be significantly reduced due to the increased drag caused by the increased density of the atmosphere at LEO altitudes following the expansion of the atmosphere during enhanced heating following a CME impact. The density of the thermosphere can soar by a factor of 50 during solar maximum, with a commensurate increase in atmospheric drag on satellites. Due to atmospheric drag, the lowest altitude above the Earth at which an object in a circular orbit can complete at least one full revolution without propulsion is approximately 150 km. Figure 1 shows the altitude decrease during the de-orbiting of the Tiangong-1 satellite during its final year of uncontrolled reentry.
  2. LEO satellites that use the Earth’s magnetic field for attitude control to ensure that the antennas of the satellite keep pointing towards the Earth, can over-adjust their attitude during a geomagnetic storm, and end up pointing away from the Earth, or use up all the fuel they have on board to make unnecessary adjustments.
  3. Satellites in orbits that intersect the Van Allen Radiation Belts can be disabled through radiation and particle impacts on their electronics.

SANSA is ramping up its ability to provide Space Weather Warnings to not only terrestrial users of technologies such as GPS, HF Communications and Power Systems but also to be able to provide satellite operators with warnings such as that which could have prevented the Starlink disaster if it had been heeded. The Regional Space Weather warning centre operated by SANSA in Hermanus will be transitioning to 24/7 operations later this year [7,8].

A graph showing Altitude above the Earth of the Tiangong-1 satellite during its final year of uncontrolled re-entry

Figure 1. Altitude above the Earth of the Tiangong-1 satellite during its final year of uncontrolled re-entry [9] Read more about satellite drag on

SANSA Space Weather Bulletin

04 Feb 2022, composed at 08:56 SAST


Solar activity is expected to be low with background X-ray flux at B-class levels. There are six sunspot regions visible on the solar disk with simple to complex magnetic configurations. There is a high probability of C-class flaring and a low probability of M-class flaring expected. The solar wind speed is expected to remain elevated and further increase due to the persisting influence of the CME and arrival high-speed stream (HSS) from coronal hole 49 (CH49). Geomagnetic activity is expected to be at unsettled levels with isolated active intervals. There is a slight chance of a G1/minor storm today due to the influence of the CME. A G1/minor storm can also be expected tomorrow (5th of February) due to the arrival of the corotating interaction region (CIR) and HSS from CH49.

Figure 2. Excerpt from the SANSA Space Weather bulletin of 4 Feb that indicated the likelihood of a G1 storm.











[9] By Phoenix7777 – Own work data

source: Announcement: On-Orbit Status Update for Tianggong-1, China Manned Space, CC BY-SA 4.0,

Daleen Fouche