Terahertz to Degrees per hour

For decades, electronics could generate frequencies up to ~100 GHz and optics could work down to ~10 THz, but the range between 0.1 and 10 THz was hard to reach from either direction. Electronic oscillators became too slow and lasers too low-energy. Only in the last 20 years have quantum cascade lasers and photoconductive antennas started closing this gap, opening new applications in imaging and spectroscopy.

Active scanners illuminate passengers with millimeter or terahertz waves (typically 0.1–1 THz), which pass through clothing but reflect off skin and dense objects. The reflected signal creates a body outline showing concealed items without ionising radiation. Because terahertz energy is about a million times weaker than an X-ray photon, it cannot break chemical bonds or damage DNA.

No. Terahertz photons carry far less energy than visible light photons and are non-ionising — they cannot knock electrons off atoms or damage DNA. At extremely high power they could heat tissue (like a microwave), but every practical terahertz imaging system operates at power levels thousands of times below any thermal threshold. You are bathed in more terahertz radiation from your own body heat than from an airport scanner.

Red light starts around 430 THz (700 nm wavelength) and violet reaches about 750 THz (400 nm). So the entire rainbow occupies roughly 430–750 THz. Infrared sits below red at 0.3–430 THz, and ultraviolet begins above violet at 750+ THz. When someone says "terahertz imaging," they mean the far-infrared end below about 10 THz — well below anything your eyes can detect.

For some applications, yes. Terahertz imaging can distinguish cancerous from healthy tissue based on water-content differences, and it does so without ionising radiation. It is already used experimentally during skin and breast cancer surgery to check tumor margins in real time. The limitation is penetration depth: terahertz waves are absorbed by water within millimeters, so they cannot image deep organs the way X-rays or MRI can.

The ISS completes one orbit (360°) in about 92 minutes, giving roughly 235°/hr — almost 16 times faster than Earth's rotation. That is why astronauts see 16 sunrises every 24 hours. At an altitude of ~408 km, the station covers about 7.66 km/s of ground track. If you could watch it from a fixed point in space, it would visibly sweep through the sky at a rate where one degree takes only about 15 seconds.

Because even tiny drift accumulates into serious navigation errors over a flight or voyage. A navigation-grade ring-laser gyroscope drifts less than 0.01°/hr; over a 10-hour flight that is only 0.1° of heading error. A cheap MEMS gyro drifting 10°/hr would accumulate 100° of error in the same time — useless for navigation. Expressing drift in °/hr makes the operational impact immediately obvious to a pilot or engineer.

Equatorial telescope mounts have a motorised right-ascension axis aligned with Earth's rotation axis. By driving that axis at exactly 15°/hr (one sidereal rate), the telescope counter-rotates against Earth's spin, keeping a star fixed in the eyepiece. Without this drive, stars would drift out of view in seconds at high magnification. Astrophotographers rely on it for long exposures without star trails.

The Moon's apparent motion has two components. It shares the sky's overall 15°/hr westward motion due to Earth's rotation. But it also orbits Earth, moving about 0.55°/hr eastward relative to the stars (360° ÷ 27.32 days ÷ 24 hr). The net effect: the Moon moves westward across the sky at roughly 14.5°/hr, which is why moonrise occurs about 50 minutes later each day.

A Foucault pendulum's swing plane rotates relative to the floor at 15° × sin(latitude) per hour. At the North Pole (90°) that is the full 15°/hr; at 45° latitude it is about 10.6°/hr; at the equator it is zero. The pendulum always swings in a fixed plane in inertial space — it is the Earth rotating underneath it. The sine factor comes from the fact that only the vertical component of Earth's angular velocity vector projects into the pendulum's swing plane. Paris (48.9°N) sees about 11.3°/hr, which is why Foucault's original 1851 demonstration took most of a day to complete a visible rotation.