If the monthly salary is $3,237.63, you can simply multiply that by 12.
$3,237.63 x 12 = $38,851.56
Hope I helped! Have a great day.
Answer:
Great Wall of China. Photo by: dowell / Getty Images. ...
Christ the Redeemer in Rio de Janeiro. Photo by: Sam Valadi via Flickr Creative Commons BY-NC-ND 2.0. ...
Machu Picchu in Peru. ...
Chichen Itza. ...
Roman Colosseum. ...
Taj Mahal in India. ...
Petra in Jordan.
Sahara Dry; Oasis
(Spring in the
desert) is the
only fertile areas
1. Along the
Mediterranean
Coast
2. Lower Nile
3. Oasis in the
desert
1. On the
Mediterranea
n Coast, they
work in
tourism
2. On the Nile
they farm
3. Near
Oasises,
Berbers are
nomadic
herders of
sheep and
goats
1. In the cities
by car and
bus.
2. On the Nile
by boat
3. In the
middle of
the desert,
they move
by
dromedary
or camel;
also use
trucks
Sahel Short grassland
south of the
Sarah; reaches
from Red Sea to
Atlantic Ocean
1. Most people live
along the rivers; the
Upper Nile in the
east and the Niger
in the west
1. Herd sheep
which causes
overgrazing
and
desertificatio
n
2. Farm:
peanuts and
millet for
cash crops
3. Subsistent
farming
4. mining urannium 1. boats on the
rivers
2. trucks, cars
on the
highways
build
through the
Sahel
3. buses in the
cities
4. Camels and
dromedaries
are still in use
Explanation:
Abstract
Most planetary systems are formed within stellar clusters, and these environments can shape their properties. This paper considers scattering encounters between solar systems and passing cluster members, and calculates the corresponding interaction cross-sections. The target solar systems are generally assumed to have four giant planets, with a variety of starting states, including circular orbits with the semimajor axes of our planets, a more compact configuration, an ultracompact state with multiple mean motion resonances, and systems with massive planets. We then consider the effects of varying the cluster velocity dispersion, the relative importance of binaries versus single stars, different stellar host masses, and finite starting eccentricities of the planetary orbits. For each state of the initial system, we perform an ensemble of numerical scattering experiments and determine the cross-sections for eccentricity increase, inclination angle increase, planet ejection, and capture. This paper reports results from over 2 million individual scattering simulations. Using supporting analytic considerations, and fitting functions to the numerical results, we find a universal formula that gives the cross-sections as a function of stellar host mass, cluster velocity dispersion, starting planetary orbital radius, and final eccentricity. The resulting cross-sections can be used in a wide variety of applications. As one example, we revisit constraints on the birth aggregate of our Solar system due to dynamical scattering and find N ≲ 104 (consistent with previous estimates).
A monsoon climate is a tropical wet climate. They are most likely to grow C. rice.