/
BepiColombo Mission This mission will BepiColombo Mission This mission will

BepiColombo Mission This mission will - PowerPoint Presentation

thegagn
thegagn . @thegagn
Follow
342 views
Uploaded On 2020-08-05

BepiColombo Mission This mission will - PPT Presentation

explore Mercury More Information Mission Objectives BepiColombo has been designed to provide the measurements necessary to study and understand the composition geophysics atmosphere magnetosphere and history of Mercury ID: 798718

mission mercury sun planet mercury mission planet sun information flyby bepicolombo return earth orbiter atmosphere spacecraft percent orbit instruments

Share:

Link:

Embed:

Download Presentation from below link

Download The PPT/PDF document "BepiColombo Mission This mission will" is the property of its rightful owner. Permission is granted to download and print the materials on this web site for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.


Presentation Transcript

Slide1

BepiColombo Mission

This mission will explore Mercury

More Information

Slide2

Mission Objectives:

BepiColombo

has been designed to provide the measurements necessary to study and understand the composition, geophysics, atmosphere, magnetosphere and history of Mercury.

More Information

Slide3

Mission Name:

The BepiColombo Mission is named after Professor Giuseppe (Bepi) Colombo from the University of Padua, Italy.

More Information

Slide4

Key Dates:

19 October 2018……….….Launch

1 May 2027…………………..End of standard mission

1 May 2028…………………..End of extended mission

More Information

Slide5

Spacecraft:

The

BepiColombo mission is based on a transfer module and two spacecraft:

The Mercury Transfer Module (MTM). It will be jettisoned on arrival

.

The

Mercury Planetary Orbiter (

MPO

) designed

to study the planet itself

.

The Mercury

Magnetospheric

Orbiter (

MMO

) designed to investigate the planet's magnetic field.

More Information

Slide6

Slide7

Instruments:

The Mercury Planetary Orbiter (MPO)

The Mercury Magnetospheric Orbiter (MMO)

More Information

Slide8

Slide9

Information on Mercury:

Mercury is the closest planet to the

Sun.

Mercury's surface temperature can reach a scorching 840 o

F

(450

o

C) during the day but can

plummet to minus

275

o

F (minus

170

o

C) at night.Mercury is the smallest planet — it is only slightly larger than Earth's

Moon

.

Since

it has no significant atmosphere to stop impacts, the planet is pockmarked with craters

.

More Information

Slide10

Information on Mercury:

Mercury’s year is 88 days and its day is

59 Earth-days. For every two orbits of the Sun, Mercury completes three rotations about its axis.

Mercury’s oval-shaped orbit is highly

elliptical.

If

one could stand on Mercury when it is nearest to the

Sun

,

the Sun

would appear more than three times as large as it does when viewed from Earth

.

More Information

Slide11

End of show

Return to slide 1

End of slide show

Slide12

Slide13

Slide14

BepiColombo Mission

BepiColombo will explore Mercury. Europe's space scientists have identified the mission as one of the most challenging long-term planetary projects, because Mercury's proximity to the Sun makes it difficult for a spacecraft to reach the planet and to survive in the harsh environment found there.

Return

Slide15

Mission Objectives:

BepiColombo

has been designed to provide the measurements necessary to study and understand the composition, geophysics, atmosphere, magnetosphere and history of Mercury. In particular, the mission has the following scientific objectives:

Investigate the origin and evolution of a planet close to the parent star

Study Mercury as a planet: its form, interior structure, geology, composition and craters

Examine Mercury's vestigial atmosphere (exosphere): its composition and dynamics

Probe

Mercury's magnetized envelope (magnetosphere): its structure and dynamics

Determine the origin of Mercury's magnetic field

Investigate polar deposits: their composition and origin

Perform a test of Einstein's theory of general relativity

Return

Slide16

Mission Name:

BepiColombo is named after Professor Giuseppe Colombo from the University of Padua, Italy, a mathematician and engineer of astonishing imagination. He was the first to see that an unsuspected resonance is responsible for Mercury's habit of rotating on its axis three times for every two revolutions it makes around the Sun.

He also suggested to NASA how to use a gravity-assist swing-by of Venus to place the Mariner 10 spacecraft in a solar orbit that would allow it to fly by Mercury three times in 1974-5.

Giuseppe (

Bepi

) Colombo, grandfather of the flyby

(1920 – 1994)

Return

Slide17

Key Dates:

19 October 2018…………..Launch

10 April 2020…………….....Earth flyby

15 October 2020…………..First Venus flyby

11 August 2021…………….Second Venus flyby

2 October 2021…………….First Mercury flyby

23 June 2022………………..Second Mercury flyby

20 June 2023………………..Third Mercury flyby

5 September 2024………..Fourth Mercury flyby

2 December 2024…………Fifth Mercury flyby

9 January 2025……………..Sixth Mercury flyby

5 December 2025………...Arrival at Mercury

14 March 2026……………..MPO in final orbit

1 May 2027…………………..End of nominal mission

1 May 2028…………………..End of extended mission

Return

Slide18

Spacecraft:

The BepiColombo mission is based on two spacecraft:The ESA-led Mercury Planetary Orbiter (

MPO) with an instrument suite of 11 experiments and instruments. It traces a lower-apocentre orbit and is designed to study the planet itself.The JAXA-led Mercury Magnetospheric Orbiter (

MMO) carrying a payload of five experiments and instruments. It follows a higher-apocentre orbit and investigates the planet's magnetic

field.

Upon arrival, they will separate and enter their own orbits around Mercury.

The Mercury Transfer Module (

MTM

) will carry the interplanetary propulsion system, with the two solar array wings. It will be jettisoned on arrival.

Return

Slide19

Instruments:

The Mercury Planetary Orbiter (MPO) will carry a sophisticated payload of 11 instruments, comprising:

CamerasSpectrometers (IR, UV, X-ray, γ-ray, neutron)RadiometerL

aser altimeterMagnetometerParticle analyzers

K

a

-band transponder

Accelerometer

The Mercury

Magnetospheric

Orbiter

(

MMO

) will

carry a payload of five advanced scientific experiments,

including:

Magnetometer

I

on spectrometer

E

lectron

energy

analyser

C

old

and energetic plasma

detectors

P

lasma

wave

analyser

Imager

Return

Slide20

Information on Mercury:

Mercury is the closest planet to the

Sun. As such, it circles the Sun faster than all the other planets.

Because the planet is so close to the Sun

, Mercury's surface temperature can reach a scorching

840

o

F

(450

o

C).

However, since this world doesn't have a real atmosphere to entrap any heat, at night temperatures can plummet to minus

275

o

F (minus 170 o C), a temperature swing of more than 1,100 o F (600

o

C), the greatest in the solar

system.

Mercury

is the smallest planet — it is only slightly larger than Earth's

Moon

. Since it has no significant atmosphere to stop impacts, the planet is pockmarked with craters

.

Return

Slide21

Information on Mercury:

Mercury

is the second densest planet after Earth, with a huge metallic core about 75 percent of the planet's diameter.

Mercury’s year is 88 days and its day is 59

Earth-days. For

every two orbits of the Sun, Mercury completes three rotations about its

axis.

Mercury’s

oval-shaped orbit is highly elliptical, taking Mercury as close as 29 million miles (47 million km) and as far as 43 million miles (70 million km) from the

Sun

. If one could stand on Mercury when it is nearest to the

Sun

,

the Sun

would appear more than three times as large as it does when viewed from Earth

.

No atmosphere: Mercury possesses an exosphere containing 42 percent oxygen, 29 percent sodium, 22 percent hydrogen, 6 percent helium, 0.5 percent potassium, with possible trace amounts of argon, carbon dioxide, water, nitrogen, xenon, krypton and neon.

Return