we are a group of highly motivated and creative science, technology and engineering students gather together from different higher institutions and we were able to form a team known as Solar Aces. Currently, we are participating in the Summer 2019, NASA L'Space Academy. In this program, our team is classified under Team-14. Our mission is to apply our science and engineering knowledge to make everyone's life safe and more efficient here on Earth and beyond.
Summer of 2019, we were part of the L'Space Mission Concept Academy. In this Academy, we were able
to make ourselves familiar with what is needed to take a design concept from an idea to understanding
all the rigorous elements needed to become a mission.
we were also given a task to prepare 22 page PDR (Preliminary Design Review) that shows what is needed to land a
Probe on Titan, Saturn's moon!
Every mission in NASA has to have a PDR.
The purpose of the PDR is to demonstrate that the preliminary design meets all system
requirements with acceptable risk and within the cost and schedule constraints
and that it establishes the basis for proceeding with detailed design.
View our PDR
Our mission was to design a Probe loaded with a variety of scientific instruments that will be used to collect scientific data. This Probe will be a secondary payload on a Titan orbiter spacecraft. While the orbiter spacecraft orbits Titan, the second-largest moon in our solar system, we will detach and descent our Probe into Titan's atmosphere and land it on one of the largest hydrocarbon lake (Kraken Mare) found on Titan. Once we successfully land the Probe on this lake, we will be expected to collect a fluid sample from the lake as well as other scientific data that will be helpful to learn more about this moon.
Saturns largest moon, Titan, is an icy world whose surface is completly obscured by a golden hazy atmosphere. Titan is the second largest moon in our solar system. Titan is bigger than Earth's moon, and larger than even the planet Mercury. This mammoth moon is the only moon in the solar system with a dense atmosphere, and it’s the only world besides Earth that has standing bodies of liquid, including rivers, lakes and seas, on its surface. Like Earth, Titan’s atmosphere is primarily nitrogen, plus a small amount of methane. It is the sole other place in the solar system known to have an earthlike cycle of liquids raining from clouds, flowing across its surface, filling lakes and seas, and evaporating back into the sky (akin to Earth’s water cycle). Titan is also thought to have a subsurface ocean of water
Titan has a radius of about 1,600 miles (2,575 kilometers), and is nearly 50 percent
wider than Earth’s moon. Titan is about 759,000 miles (1.2 million kilometers) from Saturn,
which itself is about 886 million miles (1.4 billion kilometers) from the Sun,
or about 9.5 astronomical units (AU). One AU is the distance from Earth to the Sun.
Light from the Sun takes about 80 minutes to reach Titan; because of the distance,
sunlight is about 100 times fainter at Saturn and Titan than at Earth.
Titan takes 15 days and 22 hours to complete a full orbit of Saturn. Titan is also tidally
locked in synchronous rotation with Saturn, meaning that, like Earth’s Moon,
Titan always shows the same face to the planet as it orbits.
Saturn takes about 29 Earth years to orbit the Sun (a Saturnian year),
and Saturn’s axis of rotation is tilted like Earth’s, resulting in seasons.
But Saturn’s longer year produces seasons that each last more than seven Earth years.
Since Titan orbits roughly along Saturn’s equatorial plane,
and Titan’s tilt relative to the sun is about the same as Saturn’s,
Titan’s seasons are on the same schedule as Saturn’s—seasons that last more than seven Earth years,
and a year that lasts 29 Earth years.
(2019, April 25). NASA Science, SOLAR SYSTEMS EXPLORATIONS. Retrieved from https://solarsystem.nasa.gov/moons/saturn-moons/titan/in-depth/