Solution: Student Worksheet: Satellite Venn Diagram
The finished Venn diagram should look like this.
In the listing below, the correct answer is indicated in parentheses.
- launched in 1999 (Chandra)
- will require several rocket missions to launch the entire observatory (Con-X)
- consists of four individual satellites (Con-X)
- perform detailed studies of blackholes, supernovas, dark matter, origin, evolution, and destiny of the universe (Chandra, Astro-E, and Con-X)
- launched in 2000 (Astro-E)
- more quantitative data on abundance, velocity, temperature of gas (Con-X)
- superior ability to discriminate amongst different x-rays wavelengths (Con-X and Astro-E)
- flies more than 1/3 of the way to the moon (Chandra)
- an array of 32 individual microcalorimeters (Astro-E)
- exquisitely shaped for pairs of mirrors (Chandra)
- incorporates a three stage cooling system capable of operating the array at 60 mK for about two years (Astro-E)
- will be placed 1.5 million miles from Earth (Con-X)
- images are 25x sharper than previous x-ray telescopes (Chandra)
- designed to study the universe in x-rays (Chandra, Astro-E, and Con-X)
- detects broadest range of x-ray wavelengths(Con-X)
- focusing power equivalent to the ability to read a newspaper a half a mile away (Chandra)
- focus on smaller areas which will exclude picking up signals from external medium of hot gas (Con-X)
- X-ray telescopes are one way to observe extremely hot matter with temperature of millions of degrees (Chandra, Astro-E, and Con-X)
- data collected in hours instead days (Con-X)
- observatory must be placed high above Earth's surface because Earth's atmosphere absorbs X-rays (Chandra, Astro-E, and Con-X)
- deployment of observatory commanded by woman (Chandra)
- 10X higher spectral resolution for detecting emission from Iron (Astro-E)
- collecting areas 3 square meters which will detect x-ray sources 100x fainter (Con-X)
- a high resolution X-ray spectrometer based on a microcalorimeter array, four CCD X-ray cameras, and a hard X-ray telescope (Astro-E)
- detects and images X-ray sources billions of light years away (Chandra, Astro-E, and Con-X)
Thought Questions
Each satellite represents an improvement over previous satellites. Chandra provides better imaging capabilities than previous satellites, and Astro-E provides better spectral resolution. In addition, Con-X improves spectral resolution beyond that of Astro-E.
The satellites are complementary because Chandra provides superior images, while Astro-E and Con-X provide superior spectra.
All the satellites must be placed above the Earth's atmosphere in order to study the universe in x-rays.

Teacher's Corner