Sun

The Sun is a star at the center of the Solar System. It is a nearly perfect ball of hot plasma, heated to incandescence by nuclear fusion reactions in its core. The Sun radiates this energy mainly as light, ultraviolet, and infrared radiation, and is the most important source of energy for life on Earth.

The Sun’s radius is about 695,000 kilometers (432,000 miles), or 109 times that of Earth. Its mass is about 330,000 times that of Earth, comprising about 99.86% of the total mass of the Solar System. Roughly three-quarters of the Sun’s mass consists of hydrogen (~73%); the rest is mostly helium (~25%), with much smaller quantities of heavier elements, including oxygen, carbon, neon, and iron.

There are many potential explanations for sightings. We recommend eliminating the most common and mundane before jumping to less probable conclusions or you submit a report.

Resources

Space/NASA Launches

Planned launches occur regularly all over the globe. These tracks can help identify the potential missions or launches in your area.

SpaceLaunchSchedule.com

SpaceFlightNow.com

RocketLaunch.Live

Satellite Trackers

Satellite tracking can also be done in real-time with the aid of tracking maps. They are also helpful for tracking Starlink launches.

Heavens Above

N2YO

Satellitemap.space

Spot the Station (International Space Station)

Space Weather

There are a number of sites which track solar flares, magnetic storms, asteroids, and other events which are helpful for eliminating explanations related to astronomic phenomena.

Spaceweather.com

Spaceweather.gov

Eyes on Asteroids

 

Méprises Du Ciel

French site (with English translations) with resources and examples covering the most commonly observed phenomena and explanations for UFOs.