STEREO
Sign in to saveAlso known as Solar Terrestrial Relations Observatory, Solar Terrestrial Probe 3, STP 3
STEREO (Solar TErrestrial RElations Observatory) is a solar observation mission. Two nearly identical spacecraft (STEREO-A, STEREO-B) were launched in 2006 into orbits around the Sun that cause them to respectively pull farther ahead of and fall gradually behind the Earth. This enabled stereoscopic imaging of the Sun and solar phenomena, such as coronal mass ejections.
Key facts
- Spaceflight.COSPAR_ID
- STEREO-A: STEREO-B: n
- Spaceflight.name
- STEREO
- Spaceflight.image
- Deployment of STEREO spacecraft panels (crop).jpg
- Spaceflight.image_caption
- Illustration of a STEREO spacecraft during solar array deployment
- Spaceflight.image_size
- 250px
- Spaceflight.insignia
- Stereo logo.gif
- Spaceflight.insignia_size
- 150px
- Spaceflight.insignia_caption
- Mission insignia
- Spaceflight.mission_type
- Solar observation
- Spaceflight.operator
- NASA
- Spaceflight.SATCAT
- STEREO-A: 29510 STEREO-B: 29511
- Spaceflight.mission_duration
- Planned: 2 years STEREO-A elapsed: STEREO-B final:
- Spaceflight.manufacturer
- Johns Hopkins University Applied Physics Laboratory
- Spaceflight.launch_mass
- STEREO-A: 620 kgSTEREO-B: 620 kg
- Spaceflight.power
- 475 W
- Spaceflight.launch_date
- UTC
- Spaceflight.launch_rocket
- Delta II 7925-10L
- Spaceflight.launch_site
- Cape Canaveral SLC-17B
via Wikipedia infobox
Wikidata facts
- Image
- STEREO spacecraft model 2.png
Show 1 more fact
- Commons category
- STEREO
Sources (1)
via Wikidata · CC0
~14 min read
Article
9 sectionsContents
- Mission profile
- Loss of contact with STEREO-B
- Mission benefits
- Science instrumentation
- Spacecraft subsystems
- Gallery
- See also
- References
- External links
STEREO (Solar TErrestrial RElations Observatory) is a solar observation mission. Two nearly identical spacecraft (STEREO-A, STEREO-B) were launched in 2006 into orbits around the Sun that cause them to respectively pull farther ahead of and fall gradually behind the Earth. This enabled stereoscopic imaging of the Sun and solar phenomena, such as coronal mass ejections.
Contact with STEREO-B was lost in 2014 after it entered an uncontrolled spin preventing its solar panels from generating enough power. It was briefly resumed in 2016 before being interrupted and eventually declared lost.