ku A Local Solar System Itsinda Umunyamuryango na ku A. in iyi Ikintu?
A Birenzeho Kuva: i Birenzeho na inyuma. Yet the James Webb Space Telescope, 1.5 million km beyond Earth, keeps pace with us all year round. ku a Akadomo, Rimwe Bya i Kurura Bya Kabiri na i Bya Uruziga Impuzandengo Inyuma.
in i, na Kabiri Bya Kigenga Bya.
Kureba
A Ubuhagarike “Kuba” ya: i Na::
- Bito Idirishya ku i na Ku.
- L1 and L2: two mountain passes (saddles) on either side of Earth, about 1.5 million km away. ,: A na Bidakora. Ubwoko Gitoya buri.
- 3.: ku i Bya i. , i Kuva:.
- L4 and L5: two gentle hilltops 60 degrees ahead of and behind Earth. Kuri Bidakora, i Impamvu Bya i Ihindurangano i Igice A Igikubo. They are stable, and nature fills them: Jupiter’s L4 and L5 hold more than ten thousand Trojan asteroids.
Who lives there: SOHO has watched the Sun from L1 since 1996; it sees solar storms before they reach us. Webb works around L2, where the Sun, Earth and Moon all stay on one side, behind its sunshield, keeping the telescope at about −230 °C.
Gusobanukirwa
i Ikadiri Na:, A Gitoya Igikoresho i, na i Ingaruka Bya. Byose Kureka, in Ikadiri, ni, i in Rimwe Umwaka.
For L1 and L2 the distance from the smaller body is roughly the Hill radius:
r ≈ a · ∛(m / 3M)
For the Sun and Earth: 149.6 million km × ∛(3.04 × 10⁻⁶ / 3) ≈ 1.5 million km. Solving the balance exactly gives 1.49 million km for L1 and 1.51 million km for L2.
Umunyeshuri
i -, Na: in Bya i na = m / (m), i ni
Ω(x, y) = −(1−μ)/r₁ − μ/r₂ − ½(x² + y²)
The collinear points solve ∂Ω/∂x = 0 on the x-axis (a quintic, solved numerically here); L4 and L5 form equilateral triangles with the two bodies. Linear stability analysis shows L1-L3 are always unstable, and L4/L5 are stable when μ < μ_Routh = ½(1 − √(23/27)) ≈ 0.0385. Spacecraft at L1 and L2 fly halo or Lissajous orbits around the point rather than sitting on it.
Gushaka
The Hill radius r ≈ a·∛(m/3M) gives the approximate distance of L1 and L2 from the smaller body. Compute it for the Sun and Earth (a = 149.6 million km, m/M ≈ 3.04 × 10⁻⁶). Then for Earth and the Moon (a = 384,400 km, m/M ≈ 0.0123). Where is the Earth-Moon L2 that NASA's Gateway was once planned near?
. i.
Igisubizo
3 Muhugura Ibibazo. Kuri NIBA ni i Iburyo:.
-
How far from Earth is the Sun-Earth L2 point, where the James Webb Space Telescope works?
- A 384,000 km
- B About 1.5 million km
- C 36,000 km
- D 150 million km
i
B. About 1.5 million km
-
Utudomo, Ibintu Gukusanya...?
- A L1 and L2
- B L3 gusa
- C L4 and L5
- D Ntacyo
i
C. L4 and L5 L4 and L5 are hilltops of the effective potential, but the Coriolis effect turns a drift into a slow loop around them, as long as the smaller body is less than about 1/25 of the larger one's mass.
-
Why do spacecraft at L1 and L2 still need small engine burns?
- A Utudomo: A Gitoya KURI Igihe
- B Bya
- C Asteroids
- D in
i
A. Utudomo: A Gitoya KURI Igihe
in iyi
Inkomoko
- NASA, What is a Lagrange point?
- ESA, SOHO mission (orbit around Sun-Earth L1)
- NASA, Webb's orbit at L2
- N. J. Cornish, The Lagrange Points (WMAP education, NASA GSFC)
- Minor Planet Center, Jupiter Trojans list
ni CC BY-SA 4.0.