Our Solar System
STEM Activity 7: "Solar System Scale"
Purpose: Children measure solar system object distances using astronomical units (AU) and learn how long it takes sunlight to reach each planet/object.
Supplies needed: Unobstructed space approximately 6’ X 60’. We provide the measuring tape and planet/object cards.
Age level: upper elementary school. For groups of 8-30.
Notes: One child is the Sun and other children hold a card representing a planet/object. Since children are disappointed if they do not have a card to hold, additional moon and asteroid cards were added. Math lesson on ratios for upper elementary or above.
Solar System Update
- 09/27/17: New Horizons Discoveries Keep Coming- Pluto
- 2/10/17: Astronomers Estimate That The Solar Nebula Lasted 3 To 4 Million Years. By studying the remanent magnetizations in ancient meteorites, astronomers have determined that the solar nebula — the vast of disc of gas and dust that ultimately gave rise to the solar system — lasted around 3 to 4 million years.
- 08/15/16: NASA's Van Allen Probes Catch Rare Glimpse of Supercharged Radiation Belt. Our planet is nestled in the center of two immense, concentric doughnuts of powerful radiation: the Van Allen radiation belts, which harbor swarms of charged particles that are trapped by Earth’s magnetic field. On March 17, 2015, an interplanetary shock – a shockwave created by the driving force of a coronal mass ejection, or CME, from the sun – struck Earth’s magnetic field, called the magnetosphere, triggering the greatest geomagnetic storm of the preceding decade. And NASA's Van Allen Probes were there to watch the effects on the radiation belts.
- 05/17/16: Other Suns got the right spin. Astrophysicists from the Leibniz Institute for Astrophysics Potsdam (AIP) and the Johns Hopkins University in Baltimore have for the first time measured the rotation periods of stars in a cluster nearly as old as the Sun and found them to be similar. It turns out that these stars spin around once in about twenty-six days – just like our Sun. This discovery significantly strengthens what is known as the solar-stellar connection, a fundamental principle that guides much of modern solar and stellar astrophysics.
- 05/03/16: Evidence Points to Planet Nine Existing, But How Was it Produced?. Earlier this year scientists presented evidence for Planet Nine, a Neptune-mass planet in an elliptical orbit 10 times farther from our Sun than Pluto. Since then theorists have puzzled over how this planet could end up in such a distant orbit.
- 10/27/15: SwRI scientists predict that rocky planets formed from ‘pebbles’
Southwest Research Institute scientists developed a new process in planetary formation modeling that explains the size and mass difference between the Earth and Mars.
- 10/16/15: Study questions dates for cataclysms on early moon, Earth.
New work provides surprising new details about the trigger that may have started the earliest phases of planet formation in our solar system.
- 9/24/15: 'Fossils' of Galaxies Reveal the Formation and Evolution of Massive Galaxies
An international team led by researchers at Swiss Federal Institute of Technology in Zürich observed massive dead galaxies in the universe 4 billion years after the Big Bang with the Subaru Telescope's Multi-Object InfraRed Camera and Spectrograph (MOIRCS). They discovered that the stellar content of these galaxies is strikingly similar to that of massive elliptical galaxies seen locally.
- 9/17/15: Stellar atmosphere can be used to predict the composition of rocky exoplanets
researchers from Instituto de Astrofísica e Ciências do Espaço (IA3) show that the ratio of some heavy elements in a star, like Magnesium (Mg), Silicon (Si) and Iron (Fe), have a crucial influence in the composition of rocky exoplanets.
- 8/18/15: Solar System formation don't mean a thing without that spin.
A study of zircons from a gigantic meteorite impact in South Africa casts doubt on the methods used to date lunar impacts.
- 7/23/15: Dartmouth-NASA collaboration reveals new X-ray actions. Potentially destructive high-energy electrons streak into Earth's atmosphere from space, not as Shakespeare's "gentle rain from heaven," but at velocities approaching the speed of light.