Doppler spectroscopy
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Doppler spectroscopy
Summary
Doppler spectroscopy is a method of detecting extrasolar planets[1]. It draws 181 Wikipedia views per month (method_of_detecting_extrasolar_planets category, ranking #1 of 2).[2]
Key Facts
- Doppler spectroscopy's instance of is recorded as method of detecting extrasolar planets[3].
- Doppler spectroscopy's Freebase ID is recorded as /m/02qvd94[4].
- Doppler spectroscopy's NL CR AUT ID is recorded as ph119566[5].
- Doppler spectroscopy's topic's main category is recorded as Category:Brown dwarves detected by radial velocity[6].
- Doppler spectroscopy's topic's main category is recorded as Category:Exoplanets detected by radial velocity[7].
- Doppler spectroscopy's Encyclopædia Britannica Online ID is recorded as topic/Doppler-spectroscopy[8].
- Doppler spectroscopy's Microsoft Academic ID is recorded as 2779549230[9].
- Doppler spectroscopy's Bing entity ID is recorded as 2f0fbc53-4b73-ad32-5784-d4279f436533[10].
Why It Matters
Doppler spectroscopy draws 181 Wikipedia views per month (method_of_detecting_extrasolar_planets category, ranking #1 of 2).[2] It has Wikipedia articles in 16 language editions, a strong signal of global cultural recognition.[11] It is known by 20 alternative names across languages and contexts.[12]