Loading...

Glossary term: فار

Also known as اهله

Description: در نجوم، فاز به حالت روشنایی جزئی یک قمریا سیاره نسبت به یک ناظر خاص اشاره دارد. یک منبع نور دوردست معمولاً فقط نیمی از سطح یک جسم کروی را روشن می‌کند؛ بقیه سطح در تاریکی باقی می‌ماند. به همین ترتیب، تنها حدود نیمی از سطح یک جسم کروی در دید یک ناظر دوردست قرار دارد. فاز مشخص می‌کند که کدام بخش از سطح در دید ناظر روشن می شود. این فاز با تغییر موقعیت‌های نسبی جسم، ناظر و منبع نور تغییر می‌کند.
معروف‌ترین نمونه‌ها، فازهای ماه هستند. موقعیت‌های نسبی ماه، زمین به عنوان مکان ناظر و خورشید به عنوان منبع نور، با حرکت مداری ماه به دور زمین در طول حدود یک ماه تغییر می‌کنند. بنابراین، در این مدت، یک ناظر روی زمین فازهای مختلف ماه را مشاهده خواهد کرد. فازی که در آن تمام سطح ماه که در دید ناظر است روشن باشد، "ماه کامل" نامیده می‌شود؛ زمانی که هیچ منطقه‌ای از سطح روشن دیده نمی‌شود، "ماه نو" داریم. دو فاز نیمه‌روشن به ترتیب "تربیع اول" یا "تربیع دوم" نامیده می‌شوند. روشنایی کمتر از تربیع، "هلال ماه" را تشکیل می‌دهد.

فازها همچنین در سیارات منظومه شمسی (به‌ویژه در عطارد و زهره) دیده می‌شوند و برای سامانه های فراخورشیدی نیز استنباط شده‌اند. برای ماه، حتی مناطق غیرروشن به طور کامل تاریک نیستند: آن‌ها نور بازتاب شده از زمین را منعکس می‌کنند، در پدیده‌ای که به عنوان "زمین تاب" شناخته می‌شود و اولین بار توسط لئوناردو داوینچی مستند شده است.

Related Terms:



See this term in other languages

Term and definition status: The original definition of this term in English have been approved by a research astronomer and a teacher
The translation of this term and its definition is still awaiting approval

The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".

Related Media


Venus changes from being small and almost full to being large with only a thin crescent illuminated.

A Matter of Perspective

Caption: This exquisite series of images, captured from Santo Domingo, Dominican Republic, between 17 December 2019 and 25 May 2020, shows the phases of Venus as seen from Earth. As Venus and Earth orbit the Sun, we observe different portions of Venus’s sunlit half, similar to the Moon’s phases. The sequence clearly shows Venus as distant, small, bright and gibbous in the lower frames, and ends with Venus reaching the biggest apparent size of all planets (upper frames), very close to the Sun with a small elongation, and appearing as a thin crescent. In the last frame, only 2.8% of the planet’s surface is illuminated.
Credit: Christofer Baez/IAU OAE (CC BY 4.0)

License: CC-BY-4.0 Creative Commons تخصیص 4.0 بین‌المللی (CC BY 4.0) icons


At the top Venus is full and appears small. As the images progress it moves to half, crescent and new, appearing larger.

Phases of Venus

Caption: This is a mesmerising series of images of Venus captured from Surgères, Charente-Maritime, France, over a period of six months in 2015. The phases appear similar to the phases we see of our own Moon and occur for similar reasons. Only half of Venus is illuminated by the Sun and, from Earth, we can sometimes only see part of that illuminated half, depending on the relative positions of the Sun, Earth and Venus. Both Mercury and Venus exhibit phases because their orbit is between the Sun and the orbit of Earth. Depending on the position of Venus relative to the Sun and Earth, Venus goes through its phases over a period of time. This sequence of images beautifully showcases the transition from the ‘gibbous’ to the slender crescents. The use of infrared filters helped to capture Venus's dense perpetual cloud cover during daylight in sharp detail, providing a glimpse into the mysterious nature of the planet’s atmosphere.
Credit: Stephane Gonzales/IAU OAE (CC BY 4.0)

License: CC-BY-4.0 Creative Commons تخصیص 4.0 بین‌المللی (CC BY 4.0) icons


Mercury appears smaller and fainter than Venus. The bottom right of Venus is an illuminated crescent.

Venus and Mercury Trails

Caption: In this composite image, both Mercury (left) and Venus (right) can be seen heading into the sunset. The phases of each are beautifully captured as they descend. Not all planets or moons in the Solar System show phases as viewed from Earth. This phenomenon occurs because the orbits of Venus and Mercury are positioned between Earth’s orbit and the Sun, sometimes allowing us to see only part of the illuminated portion of each planet. These phases are similar to the phases we see of our own Moon.
Credit: Marcella Giulia Pace (CC BY 4.0)

License: CC-BY-4.0 Creative Commons تخصیص 4.0 بین‌المللی (CC BY 4.0) icons