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PROGRAMA ESTRELLA

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To study the bodies that are in the frontiers of the Solar System ... taken during three hours in which the arrow shows the ubication of 2003 UB 313 ... – PowerPoint PPT presentation

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Title: PROGRAMA ESTRELLA


1
MISION ESPACIAL KUIPER
  • PROGRAMA ESTRELLA

2
PARTICIPANTS
STUDENTS
TEACHERS
3
GOALS
  • To study the bodies that are in the frontiers of
    the Solar System
  • Apply the physics knowledge while working on the
    proyect
  • To know the effects of the human body in the space

4
Where we go?
Kuipers Belt is the the group of bodies that
turn around the Sun farther than Pluto, that are
considerated as the end of the Solar System. It
is believed that the comets of short period come
out of this belt. In the last years, the objects
that are part of this zone of the Solar System
that have been studing with much interest by the
scientific community, because there have been
discovered some bodies that can be catalogued as
planets.
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2003 UB 313
We are going to 2003 UB 313 that is the closest
object of the belt, and which is called the tenth
planet because it is bigger than Pluto.
2003 UB313 was discovered by the team of Michael
Brown, Chad Trujillo y David Rabinowitz, the 18th
of January of 2005, from the images taken by the
21th of october of 2003. The discovery was
anounced on July 29 of 2005, the same day that
other two big objects of the Kuipper Belt 2003
EL61 and 2005 FY9.
Image of the telescope taken during three hours
in which the arrow shows the ubication of 2003 UB
313
7
Aproximated orbit of UB 313
8
GENERAL CHARACTERISTICS OF THE OBJECT
  • Aproximate size 2.400 km being the 16th bigger
    body size of the Solar System, somethig bigger
    than Pluto.
  • Posible natural satelites Around it turns around
    a small natural satelite S/2005 (2003 UB313)
    designated as Gabrielle.
  • Albedo Ub313 is one of the bodies that reflects
    more radiation in all the solar system, which can
    been explained by the frozen methane that covers
    all the surface.
  • Distance to the Sun The object is right now at a
    distance of 97 astronomic units and turns around
    the sun in a very inclinated and excentric orbit
    every 557 years. It is calificated as a SDO
    (Scattered disk objects).
  • Inclination of the orbit To the contrary of the
    telluric planets and the gas giants, whose orbits
    are aproximatedly in the same plane that the
    Earth, the orbit of 2003 UB313 is inclinated some
    44 according to the ecleptic.

9
SPACIAL MISSION TRIPULATED TO UB 313
10
SPACIAL VEHICLE
Shuttle Spacial vehicle reusable Shuttle with
Delta wings. 37 m long, 24 m wide 100 tonels de
basic weight Reutilization of the two lateral
rockets Exterior tank no reusable, it is
desintegrated when it comes back to the
atmosphere.
11
WORKING ON THE SHUTTLE
12
TAKE OFF ORBIT
The shuttle must be sent out with a velocity
superior to 11.7 km/s to superate the scape
velocity of the Earth,so it can scape its
gravitatory force making an hiperbolic orbit that
allows it to reach UB313.
13
OUR MISSIONS PATH
14
moment of taking off
15
UB313

Tierra
This is the moment of taking off
The shuttle must be sent in the moment that the
Earth and the asteroid UB313, in Kuippers Belt,
are at the less possible distance, which is
called the perigeus.
16
THE BEST MOMENT FOR THE LAUNCHING IS
The Earth turns around the Sun at a velocity rate
of 107.000 Km/h. If our interplanetary shuttle
is pointing the same direction in which the Earth
is already directed, it will recibe a good lift.
Even more, the Earth turns arounds toward east
over its axis, one complete turn every day. Our
planet turns around at a medium velocity of 1600
Km/h every day. So, if we send the shuttle
towards east, it will recieve a good impulse
because of the rotational movement of the Earth.
UB313 has a perhile of 35 UA, the Earth is at UA
from the Sun, then the ideal moment for the
shutting would be when the Earth and UB 313 are
at 36 UA (perigeus of UB 313)
17
How much TIME WILL IT TAKE?
  • An object at rest tends to stay at rest and an
    object in motion tends to stay in motion with the
    same speed and in the same direction unless acted
    upon by an unbalanced force. (Newtons First Law)

18
  • Most favorable distance (d) 36 UA
  • 1 UA150.000.000 Km
  • Velocity limit of scape of the Earth 11,7 Km/s
  • By the first Law of Newton we consider in an
    ideal way, that this velocity is the one that
    will mantain the shuttle during all the
    trayectory in abscense of external forces.
  • Making the adecuated calculations, we get to the
    conclusion that the journey will take
    aproximately15 years!
  • Even though, the impulse that generates the
    conditions of the launching (movement of
    traslation and rotation of the Earth) will give
    us more initial velocity and it can also save us
    some months
  • () every calculation was realized considering
    ideal conditions in which the friction of the
    terrestal atmosphere and the gravitatory
    influence of the planets that the shuttle will
    find in its path are despicable.

19
Crew
  • Three sciencist specializated in all the areas
    needed for the investigation and maintenance of
    the spaceship.
  • A copilot
  • A pilot
  • A commander, ready to do any tipe of activity
    that could do another member of the tripulation.
  • Two or three people who have knowledge on all the
    areas, including some scientific areas that the
    other crew members also know, that in case of
    emergency, they could replace the position of
    another crew member.

20
LIFE IN THE SHUTTLE
  • Physical exercise to avoid muscle atrophy
  • Time to study about the mission and its objective
  • Spare time to practise hobbies and to make
    social life with the rest of the crew
  • Communication with Earth with the mission
    control and with the crew relatives
  • Sleep time about 8 hours per day

21
WATER FILTER
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Dirty Water

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Pure Water
31
WATER SUPPLY MODEL
32
Water Course
33
H2O
H2O
H2O
Water filter
34
CO2
O2
O2
CO2
35
CH4 ENERGY SUPPLY
36
MAKING THE MODEL OF ENERGY SUPPLY
37
Space greenhouse
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39
Co2
Co2
O2
O2
40
Organic Residues (Dead plants and leaves))
41

Food
Organic Residues (Dead plants and leaves))
42
But, they need...
43
-Water -Co2 in day O2 in night -Food -Soil
44
SHOWING OUR WORK
45
WEEKS WEEKS OF WORK
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