{"id":2101,"date":"2023-04-06T18:07:16","date_gmt":"2023-04-06T15:07:16","guid":{"rendered":"https:\/\/www.blog.extremeoutdoor.com.tr\/?p=2101"},"modified":"2023-04-06T18:07:17","modified_gmt":"2023-04-06T15:07:17","slug":"astronomi-sozlugu","status":"publish","type":"post","link":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/2023\/04\/06\/astronomi-sozlugu\/","title":{"rendered":"ASTRONOM\u0130 S\u00d6ZL\u00dc\u011e\u00dc"},"content":{"rendered":"

Astronomi :<\/strong> G\u00f6kcisimlerinin \u00f6zelliklerini ve birbirleriyle ili\u015fkilerini inceleyen bilim dal\u0131.

Airy Disk Parlakl\u0131k Fakt\u00f6r\u00fc :<\/strong> Y\u0131ld\u0131zlar d\u00fcnyadan \u00e7ok uzakta olduklar\u0131 i\u00e7in teleskopla bak\u0131ld\u0131\u011f\u0131nda disk \u015feklinde de\u011fil, nokta \u015feklinde g\u00f6r\u00fcn\u00fcrler. Ancak y\u0131ld\u0131z\u0131n g\u00f6r\u00fcnt\u00fcs\u00fcn\u00fc \u00e7ok fazla b\u00fcy\u00fct\u00fcrsek teleskoptan kaynaklanan disk \u015feklinde bir g\u00f6r\u00fcnt\u00fc belirir. Yani y\u0131ld\u0131z teleskobun g\u00f6r\u00fc\u015f alan\u0131n\u0131n merkezinde oldu\u011funda, y\u0131ld\u0131z\u0131n bu b\u00fcy\u00fct\u00fclm\u00fc\u015f g\u00f6r\u00fcnt\u00fcs\u00fcnde iki \u015fey g\u00f6ze \u00e7arpmaktad\u0131r : Birincisi Airy Disk ad\u0131yla bilinen parlak bir merkezi alan, ikincisi ise K\u0131r\u0131n\u0131m halkalar\u0131 ad\u0131yla bilinen bir halka veya s\u00f6n\u00fck halkalar serisidir.

A\u00e7\u0131k k\u00fcme :<\/strong> Sarmal g\u00f6kadalar\u0131n disklerinde yer alan, y\u00fczlerce gen\u00e7 ve b\u00fcy\u00fck k\u00fctleli y\u0131ld\u0131zladan olu\u015fan gev\u015fek y\u0131ld\u0131z toplulu\u011fu.

A\u00e7\u0131kl\u0131k :<\/strong> B\u00fct\u00fcn teleskoplar\u0131n as\u0131l fonksiyonu \u0131\u015f\u0131k toplamakt\u0131r. Teleskobun a\u00e7\u0131kl\u0131\u011f\u0131 demek, merce\u011fin yada aynan\u0131n \u00e7ap\u0131 demektir. A\u00e7\u0131kl\u0131k genellikle ” (in\u00e7) ile tan\u0131mlan\u0131r. 1″ = 2.54cm dir. A\u00e7\u0131kl\u0131k ne kadar b\u00fcy\u00fckse teleskop o kadar fazla \u0131\u015f\u0131k toplar. Daha \u00e7ok \u0131\u015f\u0131k toplanmas\u0131 ise daha parlak ve daha iyi bir g\u00f6r\u00fcnt\u00fc olu\u015fmas\u0131n\u0131 sa\u011flar.

Andromeda :<\/strong> Zincirli prenses tak\u0131my\u0131ld\u0131z\u0131n\u0131n latince ad\u0131. Ayn\u0131 isim tak\u0131my\u0131ld\u0131z i\u00e7indeki g\u00f6kadam\u0131za en yak\u0131n g\u00f6kadayada ismini vermi\u015ftir.

Astroid :<\/strong> G\u00fcne\u015f sistemi’nde, \u00e7o\u011funlukla Mars ve J\u00fcpiter aras\u0131ndaki astroid ku\u015fa\u011f\u0131nda bulunan, ama baz\u0131lar\u0131 (\u00f6rne\u011fin Apollo astroidleri) D\u00fcnya’n\u0131n y\u00f6r\u00fcngesiyle kesi\u015fen y\u00f6r\u00fcngelerde ilerleyen, \u00e7aplar\u0131 \u00fc\u00e7y\u00fcz kilometre kadar olabilen kaya par\u00e7alar\u0131.

Aurora :<\/strong> Kuzey \u0131\u015f\u0131klar\u0131 olarakta bilinir. D\u00fcnya’n\u0131n manyetik alan \u00e7izgilerinin a\u00e7\u0131k oldu\u011fu kutup b\u00f6lgelerinden i\u00e7eri giren G\u00fcne\u015f kaynakl\u0131 y\u00fckl\u00fc par\u00e7ac\u0131klar\u0131n, atmosferimizdeki gazlar\u0131 \u0131\u015f\u0131tmas\u0131 sonucu olu\u015fan renkli g\u00f6r\u00fcnt\u00fcler.

Beyaz c\u00fcce :<\/strong> Y\u00fczey s\u0131cakl\u0131\u011f\u0131 yakla\u015f\u0131k 100.000 C olan, birka\u00e7 bin kilometre \u00e7ap\u0131ndaki k\u00fc\u00e7\u00fck y\u0131ld\u0131z. G\u00fcne\u015f benzeri y\u0131ld\u0131zlar\u0131n evriminin son basama\u011f\u0131d\u0131r.

Bulutsu (nebula) :<\/strong> G\u00f6ky\u00fcz\u00fcnde bulan\u0131k bir \u0131\u015f\u0131k lekesi olarak g\u00f6zlenen, g\u00f6kadam\u0131zdaki bir gaz bulutu ya da ba\u015fka bir g\u00f6kada olabilecek g\u00f6kcismi.

C\u00fcce y\u0131ld\u0131z :<\/strong> yar\u0131\u00e7ap\u0131 G\u00fcne\u015f’inkinden k\u00fc\u00e7\u00fck olan y\u0131ld\u0131z. S\u0131cakl\u0131\u011f\u0131 rengini belirler (so\u011fuk y\u0131ld\u0131zlar k\u0131rm\u0131z\u0131, s\u0131cak y\u0131ld\u0131zlar mavidir)

\u00c7\u0131k\u0131\u015f A\u00e7\u0131kl\u0131\u011f\u0131 :<\/strong> A\u00e7\u0131kl\u0131k (mm) \/ G\u00f6z merce\u011finin g\u00fcc\u00fc olarak tan\u0131mlanabilir. G\u00f6zmerce\u011finden \u00e7\u0131kan dairesel olan \u0131\u015f\u0131k demeti i\u00e7in kullan\u0131lmaktad\u0131r.

\u00c7ift y\u0131ld\u0131z sistemi :<\/strong> Birbiri \u00e7evresinde d\u00f6nen iki y\u0131ld\u0131zdan olu\u015fan sistem.

\u00c7\u00f6z\u00fcmleme :<\/strong> Bir teleskobun daha fazla ayr\u0131nt\u0131y\u0131 g\u00f6sterebilme yetene\u011fine denir. \u00c7\u00f6z\u00fcmleme ne kadar y\u00fcksekse, teleskop o kadar ince ayr\u0131nt\u0131 verir.

\u00c7\u00f6z\u00fcmleme G\u00fcc\u00fc :<\/strong> Birbirine \u00e7ok yak\u0131n olan \u00e7ift y\u0131ld\u0131zlar\u0131 ayr\u0131 ayr\u0131 g\u00f6rebilmemizi ger\u00e7ekle\u015ftiren teleskop yetene\u011fine denir.

Dev y\u0131ld\u0131z :<\/strong> Yar\u0131\u00e7ap\u0131 G\u00fcne\u015f’inkinden \u00e7ok daha b\u00fcy\u00fck olan y\u0131ld\u0131z.

Galaksi k\u00fcmeleri :<\/strong> Y\u00fczlerce ya da binlerce g\u00f6kadan\u0131n bir arada oldu\u011fu topluluklar.

Galaksi (G\u00f6kada) :<\/strong> K\u00fctlesi G\u00fcne\u015f’in k\u00fctlesinin y\u00fcz milyon kat\u0131ndan bir milyar kat\u0131na kadar olabilen dev y\u0131ld\u0131z sistemleri, \u00f6rne\u011fin Samanyolu. G\u00f6kadalar \u015fekillerine g\u00f6re elips bi\u00e7imli g\u00f6kadalar, sarmal ve d\u00fczensiz g\u00f6kadalar olmak \u00fc\u00e7 grupta toplan\u0131rlar.

Gezegen :<\/strong> G\u00fcne\u015f etraf\u0131ndaki y\u00f6r\u00fcngeleri sabit elipsler olan ve belli b\u00fcy\u00fckl\u00fcklerdeki g\u00f6kcisimleri. G\u00f6kk\u00fcre \u00fczerinde sabit nokta \u015feklinde g\u00f6r\u00fclen y\u0131ld\u0131zlardan farkl\u0131 olarak hareketli olduklar\u0131 i\u00e7in bu ad\u0131 alm\u0131\u015flard\u0131r.

Gezegenimsi bulutsu :<\/strong> K\u0131rm\u0131z\u0131 bir dev y\u0131ld\u0131z\u0131n d\u0131\u015f katmanlar\u0131n\u0131 uzaya p\u00fcsk\u00fcrtmesi sonucu olu\u015fan, merkezdeki s\u0131cak ve s\u0131k\u0131 y\u0131ld\u0131z taraf\u0131ndan ayd\u0131nlat\u0131lan gaz kabuk.

G\u00f6r\u00fc\u015f Alan\u0131 :<\/strong> Teleskop ile g\u00f6r\u00fclebilecek g\u00f6ky\u00fcz\u00fc par\u00e7as\u0131na ger\u00e7ek g\u00f6r\u00fc\u015f alan\u0131 denir. Bu a\u00e7\u0131sal alan yay derecesi cinsinden \u00f6l\u00e7\u00fcl\u00fcr. Form\u00fcl\u00fc : Teleskobun g\u00fcc\u00fc \/ G\u00f6zmerce\u011finin g\u00f6r\u00fc\u015f alan\u0131 (derece) dir.

G\u00fc\u00e7 (B\u00fcy\u00fctme) :<\/strong> Teleskobun g\u00fcc\u00fc, teleskobun kendisi ve kullan\u0131lan g\u00f6z merce\u011fi (ok\u00fcler) aras\u0131ndaki ili\u015fki olarak tan\u0131mlanabilir. Teleskop al\u0131n\u0131rken a\u00e7\u0131kl\u0131k ve teleskobun g\u00fcc\u00fcne \u00e7ok dikkat edilmelidir. B\u00fcy\u00fctme = Teleskobun odak uzakl\u0131\u011f\u0131 \/ g\u00f6zmerce\u011finin odak uzakl\u0131\u011f\u0131 form\u00fcl\u00fc ile hesaplan\u0131r. Normal \u015fartlar alt\u0131nda en y\u00fcksek b\u00fcy\u00fctme teleskobun a\u00e7\u0131kl\u0131\u011f\u0131n\u0131n 60 kat\u0131na e\u015fittir. Mesela 3.5″ lik bir teleskobun max. b\u00fcy\u00fctmesi 210X dir. Genelde amat\u00f6r astronomlar g\u00f6zlemlerinin \u00e7o\u011funu a\u00e7\u0131kl\u0131\u011f\u0131n 20-25 kat\u0131 bir b\u00fcy\u00fctme ile yaparlar.

I\u015f\u0131k Toplama G\u00fcc\u00fc :<\/strong> \u0130nsan g\u00f6z\u00fc ile teleskobun kuramsal olarak \u0131\u015f\u0131k toplama yetene\u011finin kar\u015f\u0131la\u015ft\u0131r\u0131lmas\u0131d\u0131r.

Kara delik :<\/strong> \u00c7\u00f6kerek, \u0131\u015f\u0131\u011f\u0131n bile kurtulamayaca\u011f\u0131 kadar yo\u011funla\u015fm\u0131\u015f maddenin bulundu\u011fu b\u00f6lge.

Karanl\u0131k madde :<\/strong> Varl\u0131\u011f\u0131, yayd\u0131\u011f\u0131 \u0131\u015f\u0131n\u0131m yoluyla de\u011fil de dinamik y\u00f6ntemlerle saptanabilen madde.

Kontrast :<\/strong> Elde edilen g\u00f6r\u00fcnt\u00fcn\u00fcn daha net ve daha parlak olmas\u0131d\u0131r. Kontrast\u0131n iyi olabilmesi i\u00e7in hava ve g\u00f6r\u00fc\u015f ko\u015fullar\u0131n\u0131n iyi olmas\u0131 gereklidir.

Kozmik \u0131\u015f\u0131nlar :<\/strong> G\u00fcne\u015f’te, n\u00f6tron y\u0131ld\u0131zlar\u0131nda, s\u00fcpernova patlamalar\u0131 s\u0131ras\u0131nda ya da kara deliklerde \u00fcretilen ve D\u00fcnya’ya \u0131\u015f\u0131k h\u0131z\u0131na yak\u0131n h\u0131zlarla ula\u015fan elektrik y\u00fckl\u00fc atom par\u00e7ac\u0131klar\u0131.

Kozmoloji :<\/strong> Evreni bir b\u00fct\u00fcn olarak inceleyen bilim dal\u0131.

Kuazar ( Quasar, y\u0131ld\u0131z\u0131ms\u0131 cisim ) :<\/strong> G\u00f6kada \u00e7ekirdeklerindeki, optik ve mor\u00f6tesi \u0131\u015f\u0131n\u0131m yayan s\u0131k\u0131 \u0131\u015f\u0131n\u0131m kaynaklar\u0131. Optik foto\u011fraflarda y\u0131ld\u0131z gibi g\u00f6r\u00fcn\u00fcrler. Y\u0131ld\u0131z\u0131ms\u0131 cisim g\u00fc\u00e7l\u00fc bir radyo kayna\u011f\u0131 ise kuazar olarak adland\u0131r\u0131l\u0131r.

Kuyrukluy\u0131ld\u0131z :<\/strong> G\u00fcne\u015f etraf\u0131nda \u00e7o\u011funlukla parabolik y\u00f6r\u00fcngelerde dolanan ve ufak partik\u00fcller ihtiva eden buz yap\u0131. G\u00fcne\u015fe yakla\u015ft\u0131k\u00e7a eriyen g\u00f6kcisminden arta kalan maddenin kuyruk olu\u015fturmas\u0131 ve G\u00fcne\u015f \u0131\u015f\u0131\u011f\u0131n\u0131 yans\u0131tmas\u0131 nedeniyle bu ad\u0131 alm\u0131\u015ft\u0131r.

K\u00fcresel k\u00fcmeler :<\/strong> G\u00f6kadalar\u0131n halelerinde bulunan, bir milyon ya da daha fazla say\u0131da y\u0131ld\u0131z bar\u0131nd\u0131ran, yo\u011fun y\u0131ld\u0131z topluluklar\u0131.

Messier M1-M103 :<\/strong> 18. y\u00fczy\u0131lda ya\u015fam\u0131\u015f Frans\u0131z g\u00f6kbilici Charles Messier taraf\u0131ndan derlenen bulutumsu g\u00f6kcisimleri katalogu.

Nebula (bulutsu) :<\/strong> bkz. bulutsu

N\u00f6tron y\u0131ld\u0131z\u0131 :<\/strong> Madde’nin, n\u00f6tronlar\u0131 birbirine de\u011fecek kadar s\u0131k\u0131\u015f\u0131k oldu\u011fu, yaln\u0131zca 10-20 kilometre \u00e7ap\u0131ndaki k\u00fc\u00e7\u00fck, \u00f6l\u00fc y\u0131ld\u0131z.

Odak Oran\u0131 (Foto\u011frafik H\u0131z) :<\/strong> Odak Oran\u0131 = Odak Uzakl\u0131\u011f\u0131 (mm) \/ A\u00e7\u0131kl\u0131k (mm) ile hesaplan\u0131r. Odak oran\u0131 size teleskobunuzla foto\u011fraf \u00e7ekebilme h\u0131z\u0131n\u0131 verir.

Odak Uzakl\u0131\u011f\u0131 :<\/strong> Odak uzakl\u0131\u011f\u0131 = A\u00e7\u0131kl\u0131k (mm) * Odak Oran\u0131 olarak tan\u0131mlanabilir. Ya da mercekten veya birinci aynadan itibaren teleskobun odak noktas\u0131na kadar olan uzakl\u0131\u011f\u0131d\u0131r. Odak uzakl\u0131\u011f\u0131 uzun olan teleskoplar\u0131n g\u00fcc\u00fc daha fazla olup, elde edilen g\u00f6r\u00fcnt\u00fcde daha b\u00fcy\u00fckt\u00fcr.

Ok\u00fcler (g\u00f6z merce\u011fi) : <\/strong>Teleskopta olu\u015fturulan g\u00f6r\u00fcnt\u00fcler, farkl\u0131 oranlarda g\u00f6zmercekleri taraf\u0131ndan b\u00fcy\u00fct\u00fcl\u00fcrler.

Optik Dizayn Sap\u0131n\u00e7lar\u0131 :<\/strong> G\u00f6r\u00fcnt\u00fcn\u00fcn olu\u015fumu s\u0131ras\u0131nda ortaya \u00e7\u0131kan hatalara denir. Renk sap\u0131nc\u0131, K\u00fcresel sap\u0131n\u00e7, Koma, Astigmat, Alan e\u011frili\u011fi ve Alan bozulmas\u0131 baz\u0131 teleskop sap\u0131n\u00e7lar\u0131d\u0131r.

Parlakl\u0131k S\u0131n\u0131r\u0131 :<\/strong> Parlakl\u0131k birimi kadir (m) dir. 7.5 + 5 * logA (cm biriminde teleskobun a\u00e7\u0131kl\u0131\u011f\u0131n\u0131n logaritmas\u0131) form\u00fcl\u00fc ile g\u00f6rsel parlakl\u0131k s\u0131n\u0131r\u0131 hesaplan\u0131r.

Pulsar :<\/strong> H\u0131zla d\u00f6nen, g\u00fc\u00e7l\u00fc manyetik alana sahip n\u00f6tron y\u0131ld\u0131z\u0131 yap\u0131s\u0131nda olan ve atmalar halinde radyo dalgalar\u0131 yayan kaynak.

Radyoteleskop :<\/strong> G\u00f6kcisimlerini ara\u015ft\u0131rmak i\u00e7in kullan\u0131lan uzun dalgaboyuna duyarl\u0131 alet.

Salma \u00e7izgisi :<\/strong> Bir kayna\u011f\u0131n tayf\u0131ndaki, belirli bir elementin atomlar\u0131n\u0131n belirli bir dalga boyundaki \u0131\u015f\u0131k salmas\u0131ndan kaynaklanan parlak \u00e7izgi.

Samanyolu :<\/strong> S\u00fct yolu olarakta bilinir. \u0130\u00e7inde bulundu\u011fumuz g\u00f6kada. G\u00f6zlemsel astronomide g\u00f6ky\u00fcz\u00fcnde \u015ferit halinde g\u00f6r\u00fclen bulutsu yap\u0131. (asl\u0131nda g\u00f6r\u00fclen g\u00f6kadam\u0131z\u0131n bir koludur)

So\u011furma \u00e7izgisi :<\/strong> Ayn\u0131 tayftaki karanl\u0131k \u00e7izgi.

S\u00fcperdev :<\/strong> I\u015f\u0131ma g\u00fcc\u00fc \u00e7ok y\u00fcksek olan dev y\u0131ld\u0131z.

S\u00fcpernova :<\/strong> Y\u0131ld\u0131z evriminin bir basama\u011f\u0131nda; y\u0131ld\u0131z\u0131n i\u00e7erdi\u011fi maddeyi uzaya f\u0131rlatmas\u0131yla sonu\u00e7lanan b\u00fcy\u00fck patlamalar.

Quasar :<\/strong> bkz. Kuasar

Tak\u0131my\u0131ld\u0131z :<\/strong> Bak\u0131\u015f do\u011frultumuza g\u00f6re bir toplulukmu\u015f gibi g\u00f6r\u00fcnen, g\u00f6ky\u00fcz\u00fcnde belirgin \u015fekiller olu\u015fturan y\u0131ld\u0131zlar toplulu\u011fu.

Tayf :<\/strong> Bir kaynaktan gelen \u0131\u015f\u0131\u011f\u0131n, \u00f6rne\u011fin bir prizma yard\u0131myla \u00e7e\u015fitli dalga boylar\u0131na ayr\u0131lmas\u0131. Ya\u011fmur damlalar\u0131 prizma etkisi yaparak g\u00fcne\u015fin tayf\u0131n\u0131 g\u00f6kku\u015fa\u011f\u0131 \u015feklinde g\u00f6sterirler.

Tutulum :<\/strong> D\u00fcnya \u00e7evresinde d\u00f6nerken, G\u00fcne\u015f’in bir y\u0131l i\u00e7inde g\u00f6ky\u00fcz\u00fcnde izler gibi g\u00f6r\u00fcnd\u00fc\u011f\u00fc b\u00fcy\u00fck \u00e7ember. Tutulum d\u00fczlemi, D\u00fcnya’n\u0131n y\u00f6r\u00fcnge d\u00fczlemidir.

Uydu :<\/strong> Bir g\u00f6kcisminin \u00e7ekim alan\u0131 nedeniyle belli bir y\u00f6r\u00fcngeye oturmu\u015f cisim. Yapay uydular D\u00fcnya etraf\u0131nda dolan\u0131r. Ayda D\u00fcnya’n\u0131n uydusudur.

Yak\u0131n Odak :<\/strong> G\u00f6rsel veya foto\u011frafik \u00e7al\u0131\u015f\u0131labilecek en yak\u0131n yer cisminin odaklanabilece\u011fi en yak\u0131n uzakl\u0131kt\u0131r.

Y\u0131ld\u0131z :<\/strong> \u00c7ekirdeklerindeki n\u00fckleer tepkimeler sonunda enerji yayan b\u00fcy\u00fck k\u00fctleli g\u00f6kcisimleri.

Zodyak \u0131\u015f\u0131\u011f\u0131 :<\/strong> G\u00fcne\u015f \u0131\u015f\u0131\u011f\u0131n\u0131n G\u00fcne\u015f sistemine da\u011f\u0131lm\u0131\u015f toz par\u00e7ac\u0131klar\u0131 taraf\u0131ndan sa\u00e7\u0131lmas\u0131 sonucunda bur\u00e7lar ku\u015fa\u011f\u0131n\u0131 boyunca ortaya \u00e7\u0131kan \u0131\u015f\u0131k ku\u015fa\u011f\u0131.<\/p>\n\n

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\n Oylama Yap<\/span>\n <\/div>\n <\/div>\n","protected":false},"excerpt":{"rendered":"

Astronomi : G\u00f6kcisimlerinin \u00f6zelliklerini ve birbirleriyle ili\u015fkilerini inceleyen bilim dal\u0131. Airy Disk Parlakl\u0131k Fakt\u00f6r\u00fc : Y\u0131ld\u0131zlar d\u00fcnyadan \u00e7ok uzakta olduklar\u0131 i\u00e7in teleskopla…<\/p>\n","protected":false},"author":990005,"featured_media":2102,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[16],"tags":[],"class_list":["post-2101","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-teknoloji"],"_links":{"self":[{"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/posts\/2101","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/users\/990005"}],"replies":[{"embeddable":true,"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/comments?post=2101"}],"version-history":[{"count":1,"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/posts\/2101\/revisions"}],"predecessor-version":[{"id":2103,"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/posts\/2101\/revisions\/2103"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/media\/2102"}],"wp:attachment":[{"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/media?parent=2101"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/categories?post=2101"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/blog.extremeoutdoor.com.tr\/index.php\/wp-json\/wp\/v2\/tags?post=2101"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}