Noun:

সৌর অয়নবৃত্ত, সূর্যের বার্ষিক পরিক্রমণ-পথ, ক্রাঁতিবলয়, ক্রাঁতি, গ্রহণরেখা, অয়নবৃত্ত, ক্রাঁতিবৃত্ত,

ecliptic শব্দের বাংলা অর্থ এর উদাহরণ:

প্রাচীন ব্যাবিলনবাসীরা অয়নবৃত্ত বরাবর বৃহস্পতি গ্রহের গতির সমাকলনে ট্রাপিজয়ডাল পদ্ধতি ব্যবহার করত ।

কক্ষীয় পর্যায়কাল ৭.১৫৪৫৫২৯৬d গড় কক্ষীয় দ্রুতি ১০.৮৮০km/s নতি ২.২১৪° (গ্রহণরেখা) ০.২০° (বৃহস্পতির নিরক্ষীয় অঞ্চলে) যার উপগ্রহ বৃহস্পতি গ্রহ ভৌত বৈশিষ্ট্যসমূহ ।

বর্তমানে অয়নাংশ বলতে নাক্ষত্রিক অয়নবৃত্ত, ক্রান্তীয় অয়নবৃত্ত এর চেয়ে কতটা কম ।

অয়নবৃত্ত পশ্চিম থেকে পূর্ব দিক বরাবর ২৭টি নক্ষত্রে ভাগ করা হয়েছে ।

ecliptic's Usage Examples:

path along the ecliptic against the background of stars.

The ecliptic is an important reference plane and is the basis of the ecliptic coordinate system.

approximately 8° north or south (as measured in celestial latitude) of the ecliptic, the apparent path of the Sun across the celestial sphere over the course.

Earth's orbit, called the ecliptic plane.

There are two principal variants of the ecliptic coordinate system: geocentric ecliptic coordinates centered on.

It spans 210°–240° ecliptic longitude.

The ecliptic coordinate system is a celestial coordinate system commonly used for representing the apparent positions, orbits, and pole orientations of.

orbit of the Moon intersects the ecliptic.

The ascending (or north) node is where the Moon moves into the northern ecliptic hemisphere, while the descending.

known as the ecliptic plane, and Earth's tilt is known to astronomers as the obliquity of the ecliptic, being the angle between the ecliptic and the celestial.

as the period of time for the mean ecliptic longitude of the Sun to increase by 360 degrees.

Since the Sun's ecliptic longitude is measured with respect.

moved westward along the ecliptic relative to the fixed stars, opposite to the yearly motion of the Sun along the ecliptic.

orbital plane (the plane of the ecliptic) but currently makes an angle of about 23.

44° (called the obliquity of the ecliptic), and because the axis keeps.

celestial sphere at which the ecliptic intersects the celestial equator.

Although there are two intersections of the ecliptic with the celestial equator.

from most satellites of other planets in that its orbit is close to the ecliptic plane instead of to its primary's (in this case, Earth's) equatorial plane.

ecliptic and equator increases by about 3.

1 minutes per century, but for fixed stars further from the ecliptic the.

astrology, they refer to two different systems of ecliptic coordinates used to divide the ecliptic into twelve "signs".

and latitude and other astronomically important features, such as the ecliptic.

For heliocentric orbits, the ecliptic as the reference plane, and the First Point of Aries as the origin of longitude.

Aspects are measured by the angular distance in degrees and minutes of ecliptic longitude between two points, as viewed from Earth.

with a slightly greater inclination to the ecliptic than the moon and planets.

As seen from Mars, the ecliptic (apparent plane of the sun and also the average.

objects or spacecraft have either the same right ascension or the same ecliptic longitude, usually as observed from Earth.

The ecliptic coordinate system specifies positions relative to the ecliptic (Earth's orbit), using ecliptic longitude and latitude.

Synonyms:

great circle;