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O 8

Oxygen (O)

nonmetal
Periode: 2 Golongan: 16 Blok: p

Gas

Bobot Atom Standar

15,999 u [15,99903, 15,99977]

Konfigurasi elektron

[He] 2s2 2p4

Titik lebur

-218,79 °C

Titik didih

-182,95 °C

Massa jenis

1,429 kg/m³

Bilangan oksidasi

−2, −1, 0, +1, +2

Keelektronegatifan (Pauling)

3,44

Energi ionisasi (ke-1)

13,618055 eV

Tahun penemuan

1771

Jari-jari atom

60 pm

Detail

Asal nama Greek: oxys and genes, (acid former).
Negara penemuan England/Sweden
Penemu Joseph Priestly, Carl Wilhelm Scheele

Oxygen is a reactive nonmetal and chalcogen that occurs mainly as the diatomic gas O₂ and, less commonly, as ozone O₃. It is essential to aerobic respiration and is a major constituent of water, silicate minerals, carbonates, and many biological molecules. Its high electronegativity and ability to form strong bonds make oxidation chemistry central to combustion, corrosion, metabolism, and industrial processing.

The gas is colorless, odorless, and tasteless. The liquid and solid forms are a pale blue color and are strongly paramagnetic.

The name derives from the Greek oxys for "acid" and genes for "forming" because the French chemist Antoine-Laurent Lavoisier once thought that oxygen was integral to all acids.

Oxygen was discovered independently by the Swedish pharmacist and chemist Carl-Wilhelm Scheele in 1771, and the English clergyman and chemist Joseph Priestley in 1774. Scheele's Chemical Treatise on Air and Fire was delayed in publication until 1777, so Priestley is credited with the discovery because he published first.

Oxygen had been produced by several chemists prior to its discovery in 1774, but they failed to recognize it as a distinct element. Joseph Priestley and Carl Wilhelm Scheele both independently discovered oxygen, but Priestly is usually given credit for the discovery. They were both able to produce oxygen by heating mercuric oxide (HgO). Priestley called the gas produced in his experiments 'dephlogisticated air' and Scheele called his 'fire air'. The name oxygen was created by Antoine Lavoisier who incorrectly believed that oxygen was necessary to form all acids. Oxygen is the third most abundant element in the universe and makes up nearly 21% of the earth's atmosphere. Oxygen accounts for nearly half of the mass of the earth's crust, two thirds of the mass of the human body and nine tenths of the mass of water. Large amounts of oxygen can be extracted from liquefied air through a process known as fractional distillation. Oxygen can also be produced through the electrolysis of water or by heating potassium chlorate (KClO3).

From the Greek word oxys, acid, and genes, forming. The behavior of oxygen and nitrogen as components of air led to the advancement of the phlogiston theory of combustion, which captured the minds of chemists for a century.

Joseph Priestley is generally credited with its discovery, although Scheele also discovered it independently.

Its atomic weight was used as a standard of comparison for each of the other elements until 1961 when the International Union of Pure and Applied Chemistry adopted carbon 12 as the new basis.

Gambar

Sifat

Fisika

Jari-jari atom (empiris)
60 pm Bandingkan Jari-jari atom (empiris) semua unsur →
Jari-jari kovalen
66 pm Bandingkan Jari-jari kovalen semua unsur →
Jari-jari van der Waals
152 pm Bandingkan Jari-jari van der Waals semua unsur →
Massa jenis
1,429 kg/m³ Bandingkan Massa jenis semua unsur →
Volume molar
0,014 L/mol
Fase pada STP
Gas Bandingkan Fase pada STP semua unsur →
Titik lebur
-218,79 °C Bandingkan Titik lebur semua unsur →
Titik didih
-182,95 °C Bandingkan Titik didih semua unsur →
Konduktivitas termal
0,027 W/(m·K) Bandingkan Konduktivitas termal semua unsur →
Kapasitas kalor spesifik
0,918 J/(g·K) Bandingkan Kapasitas kalor spesifik semua unsur →
Kapasitas kalor molar
29,378 J/(mol·K) Bandingkan Kapasitas kalor molar semua unsur →
Struktur kristal
Kubik Bandingkan Struktur kristal semua unsur →

Kimia

Keelektronegatifan (Pauling)
3,44 Bandingkan Keelektronegatifan (Pauling) semua unsur →
Keelektronegatifan (Allen)
3,61
Afinitas elektron
1,4611 eV
Energi ionisasi (ke-1)
13,618055 eV Bandingkan Energi ionisasi (ke-1) semua unsur →
Energi ionisasi (ke-2)
35,121241 eV Bandingkan Energi ionisasi (ke-2) semua unsur →
Energi ionisasi (ke-3)
54,935729 eV Bandingkan Energi ionisasi (ke-3) semua unsur →
Energi ionisasi (ke-4)
77,413766 eV Bandingkan Energi ionisasi (ke-4) semua unsur →
Energi ionisasi (ke-5)
113,899392 eV Bandingkan Energi ionisasi (ke-5) semua unsur →
Bilangan oksidasi
−2, −1, 0, +1, +2 Bandingkan Bilangan oksidasi semua unsur →
Elektron valensi
6 Bandingkan Elektron valensi semua unsur →
Konfigurasi elektron
[He] 2s2 2p4

Termodinamika

Titik tripel (suhu)
-218,7916 °C
Titik tripel (tekanan)
146,3 Pa
Titik kritis (suhu)
-118,569 °C
Titik kritis (tekanan)
5,043e+6 Pa
Kalor peleburan
0,00460175 eV Bandingkan Kalor peleburan semua unsur →
Kalor penguapan
0,07068456 eV Bandingkan Kalor penguapan semua unsur →
Kalor atomisasi
2,582474 eV
Entalpi atomisasi
2,583085 eV

Nuklir

Proton
8 Bandingkan Proton semua unsur →
Neutron
8 Bandingkan Neutron semua unsur →
Isotop yang diketahui
18 Bandingkan Isotop yang diketahui semua unsur →
Isotop stabil
3 Bandingkan Isotop stabil semua unsur →
Isotop paling stabil
O-16
Tahun penemuan
1771

Kelimpahan

Kelimpahan (kerak Bumi)
4,61e+5 mg/kg Bandingkan Kelimpahan (kerak Bumi) semua unsur →
Kelimpahan (samudra)
8,57 × 105 mg/L Bandingkan Kelimpahan (samudra) semua unsur →

Struktur Kristal

Konstanta kisi a
683 pm

Struktur Elektronik

Elektron per kulit
2, 6 Bandingkan Elektron per kulit semua unsur →

Pengenal

Nomor CAS
7782-44-7 Bandingkan Nomor CAS semua unsur →
Simbol term
3P2
InChI
InChI=1S/O
Kunci InChI
QVGXLLKOCUKJST-UHFFFAOYSA-N

Konfigurasi Elektron Diukur

Muatan ion
Proton 8
Elektron 8
Muatan Netral
Konfigurasi O: 2s² 2p⁴
Konfigurasi elektron
Diukur
[He] 2s² 2p⁴
1s² 2s² 2p⁴
Diagram orbital
1s
2/2
2s
2/2
2p
4/6 2↑
Total elektron: 8 Tidak berpasangan: 2 ?

Model atom

Proton 8
Neutron 8
Elektron 8
Nomor massa 16
Kestabilan Stabil

Isotop mengubah jumlah neutron, massa, dan kestabilan — bukan konfigurasi elektron atom netral.

Model atom skematis, tidak sesuai skala.

Sidik Jari Atom

Spektrum Emisi / Absorpsi

25 / 50 (50 50 dengan intensitas)
Diukur
Emisi Tampak: 380–750 nm

Distribusi Isotop

1699,7570%180,2050%170,0380%Nomor massaKelimpahan alami (%)
Nomor massaMassa atom (u)Kelimpahan alamiWaktu paruh
16 Stabil15,99491461957 ± 0,0000000001799,7570%Stabil
17 Stabil16,9991317565 ± 0,000000000690,0380%Stabil
18 Stabil17,99915961286 ± 0,000000000760,2050%Stabil
Diukur

Fase / Wujud

1 atm / 101.325 kPa
Gas 25 °C (298,15 K)

Alasan: 207,9 °C di atas titik didih (-182,95 °C)

Titik lebur -218,79 °C
Titik didih -182,95 °C
Di atas titik didih sebesar 207,9 °C
0 K Suhu saat ini: 25 °C 6000 K
Linimasa fase

Skematis, tidak sesuai skala

Padat
Cair
Gas
Peleburan
Pendidihan
25°C
Padat
Cair
Gas
Saat ini

Titik transisi fase

Titik lebur Literatur
-218,79 °C
Titik didih Literatur
-182,95 °C
Fase saat ini Dihitung
Gas

Energi transisi

Kalor peleburan Literatur
0,00460175 eV

Energi yang diperlukan untuk meleburkan 1 mol pada titik lebur

Kalor penguapan Literatur
0,07068456 eV

Energi yang diperlukan untuk menguapkan 1 mol pada titik didih

Massa jenis

Massa jenis referensi Literatur
1,429 kg/m³

Pada kondisi standar

Massa jenis saat ini Diperkirakan
0,65396019 kg/m³

Diperkirakan menggunakan hukum gas ideal pada T saat ini

Lanjutan

Titik tripel Literatur
-218,7916 °C
Titik kritis Literatur
-118,569 °C

Spektrum Atom

Data Garis Spektrum ?

IonMuatanTotal garisProbabilitas transisiPenamaan tingkat energi
O I 0910854907
O II +116308761630
O III +21005974974
O IV +3152515211523
O V +4391385385
O VI +5157126157
O VII +6189188189
O VIII +7137137137
Data Garis Spektrum NIST →

Data Tingkat Energi ?

IonMuatanTingkat energi
O I 0614
O II +1287
O III +2188
O IV +3219
O V +4172
O VI +5148
O VII +6149
O VIII +7149
Data Tingkat Energi NIST →
8 O 15.9994

Oxygen — Visualisasi Orbital Atom

[He]2s22p4
Tingkat energi 2 6
Bilangan oksidasi -2, -1, 0, +1, +2
HOMO 2p n=2 · l=1 · m=-1
Oxygen — Pratinjau Visualisasi Orbital Atom
Three.js hanya dimuat saat diminta
8 O 15.9994

Oxygen — Visualisasi Struktur Kristal

Primitive Cubic · Pearson cP1
Eksperimental
Pearson cP1
No. Koord. 6
Pengemasan 52.000%
Tidak memiliki struktur kristal pada kondisi standar — gas pada 298 K, 1 atm
Struktur fase padat pada 293 K
Oxygen — Pratinjau Visualisasi Struktur Kristal
Three.js hanya dimuat saat diminta

Jari-jari Ion

MuatanKoordinasiSpinJari-jari
-22Tidak tersedia135 pm
-23Tidak tersedia136 pm
-24Tidak tersedia138 pm
-26Tidak tersedia140 pm
-28Tidak tersedia142 pm

Senyawa

O
15,999 u
O-2
15,999 u
O-
15,999 u
O-2
17,999 u
O-2
15,003 u

Isotop (3)

Oxygen has nine isotopes. Natural oxygen is a mixture of three isotopes.

Nomor massaMassa atom (u)Kelimpahan alamiWaktu paruhMode peluruhan
16 Stabil15,99491461957 ± 0,0000000001799,7570% ± 0,0160%Stabil
stable
17 Stabil16,9991317565 ± 0,000000000690,0380% ± 0,0010%Stabil
stable
18 Stabil17,99915961286 ± 0,000000000760,2050% ± 0,0140%Stabil
stable
16 Stabil
Massa atom (u) 15,99491461957 ± 0,00000000017
Kelimpahan alami 99,7570% ± 0,0160%
Waktu paruh Stabil
Mode peluruhan
stable
17 Stabil
Massa atom (u) 16,9991317565 ± 0,00000000069
Kelimpahan alami 0,0380% ± 0,0010%
Waktu paruh Stabil
Mode peluruhan
stable
18 Stabil
Massa atom (u) 17,99915961286 ± 0,00000000076
Kelimpahan alami 0,2050% ± 0,0140%
Waktu paruh Stabil
Mode peluruhan
stable

Garis Spektrum

Menampilkan 50 dari 1013. Secara bawaan, hanya garis spektrum dengan intensitas terukur yang ditampilkan.

Panjang gelombang (nm)IntensitasTahap ionisasiJenisTransisiAkurasiSumber
615.8187 nm490O Iemission2s2.2p3.(4S*).3p 5P → 2s2.2p3.(4S*).4d 5D*DiukurNIST
615.6778 nm450O Iemission2s2.2p3.(4S*).3p 5P → 2s2.2p3.(4S*).4d 5D*DiukurNIST
700.223 nm450O Iemission2s2.2p3.(4S*).3p 3P → 2s2.2p3.(4S*).4d 3D*DiukurNIST
725.4448 nm450O Iemission2s2.2p3.(4S*).3p 3P → 2s2.2p3.(4S*).5s 3S*DiukurNIST
615.5971 nm400O Iemission2s2.2p3.(4S*).3p 5P → 2s2.2p3.(4S*).4d 5D*DiukurNIST
645.5977 nm400O Iemission2s2.2p3.(4S*).3p 5P → 2s2.2p3.(4S*).5s 5S*DiukurNIST
725.4154 nm400O Iemission2s2.2p3.(4S*).3p 3P → 2s2.2p3.(4S*).5s 3S*DiukurNIST
645.4444 nm360O Iemission2s2.2p3.(4S*).3p 5P → 2s2.2p3.(4S*).5s 5S*DiukurNIST
700.1922 nm360O Iemission2s2.2p3.(4S*).3p 3P → 2s2.2p3.(4S*).4d 3D*DiukurNIST
645.3602 nm320O Iemission2s2.2p3.(4S*).3p 5P → 2s2.2p3.(4S*).5s 5S*DiukurNIST
725.4531 nm320O Iemission2s2.2p3.(4S*).3p 3P → 2s2.2p3.(4S*).5s 3S*DiukurNIST
715.6701 nm210O Iemission2s2.2p3.(2D*).3s 1D* → 2s2.2p3.(2D*).3p 1DDiukurNIST
396.1573 nm200O IIIemission2s2.2p.(2P*).3p 1D → 2s2.2p.(2P*).3d 1F*DiukurNIST
533.0741 nm190O Iemission2s2.2p3.(4S*).3p 5P → 2s2.2p3.(4S*).5d 5D*DiukurNIST
604.6438 nm190O Iemission2s2.2p3.(4S*).3p 3P → 2s2.2p3.(4S*).6s 3S*DiukurNIST
394.72949 nm185O Iemission2s2.2p3.(4S*).3s 5S* → 2s2.2p3.(4S*).4p 5PDiukurNIST
394.74813 nm160O Iemission2s2.2p3.(4S*).3s 5S* → 2s2.2p3.(4S*).4p 5PDiukurNIST
532.9681 nm160O Iemission2s2.2p3.(4S*).3p 5P → 2s2.2p3.(4S*).5d 5D*DiukurNIST
604.6233 nm160O Iemission2s2.2p3.(4S*).3p 3P → 2s2.2p3.(4S*).6s 3S*DiukurNIST
394.75862 nm140O Iemission2s2.2p3.(4S*).3s 5S* → 2s2.2p3.(4S*).4p 5PDiukurNIST
543.6862 nm135O Iemission2s2.2p3.(4S*).3p 5P → 2s2.2p3.(4S*).6s 5S*DiukurNIST
559.789 nm130O Vemission1s2.2s.3p 3P* → 1s2.2s.3d 3DDiukurNIST
650.024 nm130O Vemission1s2.2p.(2P*<3/2>).3p 3D → 1s2.2p.(2P*<3/2>).3d 3F*DiukurNIST
382.34136 nm120O Iemission2s2.2p3.(2D*).3s 3D* → 2s2.2p3.(2P*).3p 3DDiukurNIST
557.7339 nm120O Iemission2s2.2p4 1D → 2s2.2p4 1SDiukurNIST
543.5775 nm110O Iemission2s2.2p3.(4S*).3p 5P → 2s2.2p3.(4S*).6s 5S*DiukurNIST
559.2252 nm110O IIIemission2s2.2p.(2P*).3s 1P* → 2s2.2p.(2P*).3p 1PDiukurNIST
604.6495 nm110O Iemission2s2.2p3.(4S*).3p 3P → 2s2.2p3.(4S*).6s 3S*DiukurNIST
395.46067 nm100O Iemission2s2.2p3.(4S*).3p 3P → 2s2.2p3.(2P*).3s 3P*DiukurNIST
412.396 nm100O Vemission1s2.2p.(2P*<3/2>).3s 3P* → 1s2.2p.(2P*<3/2>).3p 3DDiukurNIST
436.8258 nm100O Iemission2s2.2p3.(4S*).3s 3S* → 2s2.2p3.(4S*).4p 3PDiukurNIST
543.5178 nm90O Iemission2s2.2p3.(4S*).3p 5P → 2s2.2p3.(4S*).6s 5S*DiukurNIST
423.3274 nm80O Iemission2s2.2p3.(4S*).4p 3P → 2s2.2p3.(2D*<3/2>).3d 3P*DiukurNIST
441.4899 nm27O IIemission2s2.2p2.(3P).3s 2P → 2s2.2p2.(3P).3p 2D*DiukurNIST
672.1388 nm26O IIemission2s2.2p2.(3P).3s 2P → 2s2.2p2.(3P).3p 2S*DiukurNIST
441.6975 nm25O IIemission2s2.2p2.(3P).3s 2P → 2s2.2p2.(3P).3p 2D*DiukurNIST
397.3256 nm24O IIemission2s2.2p2.(3P).3s 2P → 2s2.2p2.(3P).3p 2P*DiukurNIST
407.58617 nm24O IIemission2s2.2p2.(3P).3p 4D* → 2s2.2p2.(3P).3d 4FDiukurNIST
464.91347 nm24O IIemission2s2.2p2.(3P).3s 4P → 2s2.2p2.(3P).3p 4D*DiukurNIST
664.1031 nm24O IIemission2s2.2p2.(3P).3s 2P → 2s2.2p2.(3P).3p 2S*DiukurNIST
407.21525 nm23O IIemission2s2.2p2.(3P).3p 4D* → 2s2.2p2.(3P).3d 4FDiukurNIST
434.9426 nm23O IIemission2s2.2p2.(3P).3s 4P → 2s2.2p2.(3P).3p 4P*DiukurNIST
411.92165 nm22O IIemission2s2.2p2.(3P).3p 4P* → 2s2.2p2.(3P).3d 4DDiukurNIST
459.0974 nm22O IIemission2s2.2p2.(1D).3s 2D → 2s2.2p2.(1D).3p 2F*DiukurNIST
464.18103 nm22O IIemission2s2.2p2.(3P).3s 4P → 2s2.2p2.(3P).3p 4D*DiukurNIST
689.5102 nm22O IIemission2s2.2p2.(3P).3d 4F → 2s2.2p2.(3P).4p 4D*DiukurNIST
406.98819 nm21O IIemission2s2.2p2.(3P).3p 4D* → 2s2.2p2.(3P).3d 4FDiukurNIST
435.126 nm21O IIemission2s2.2p2.(1D).3s 2D → 2s2.2p2.(1D).3p 2D*DiukurNIST
466.16324 nm21O IIemission2s2.2p2.(3P).3s 4P → 2s2.2p2.(3P).3p 4D*DiukurNIST
470.5346 nm21O IIemission2s2.2p2.(3P).3p 2D* → 2s2.2p2.(3P).3d 2FDiukurNIST

Sifat Lanjutan

Jari-jari Kovalen (Lanjutan)

Jari-jari kovalen (Pyykkö)
63 pm
Jari-jari kovalen (Pyykkö, ikatan rangkap dua)
57 pm
Jari-jari kovalen (Pyykkö, ikatan rangkap tiga)
53 pm
Jari-jari kovalen (Bragg)
65 pm

Jari-jari van der Waals

Bondi
152 pm
Batsanov
155 pm
Alvarez
150 pm
UFF
350 pm
MM3
182 pm
Dreiding
340,46 pm
Rowland–Taylor
158 pm

Jari-jari Atom & Logam

Jari-jari atom (Rahm)
171 pm

Skala Penomoran

Mendeleev
99
Pettifor
101
Glawe
97

Skala Keelektronegatifan

Ghosh
0
Gunnarsson–Lundqvist
8
Robles–Bartolotti
6

Polarizabilitas & Dispersi

Polarizabilitas dipol
5,3 a.u.
Polarizabilitas dipol (ketidakpastian)
0,2 a.u.
C₆
15,6 Ha·Bohr6
C₆ (Gould–Bučko)
16,7 Ha·Bohr6

Afinitas Kimia

Afinitas proton
485,2 kJ/mol
Kebasaan fase gas
459,6 kJ/mol

Transisi Fase & Alotrop

Titik lebur54,36 K
Titik didih90,19 K
Titik kritis (suhu)154,58 K
Titik kritis (tekanan)5,04 MPa
Titik tripel (suhu)54,36 K
Titik tripel (tekanan)0,15 kPa

Kategori Bilangan Oksidasi

−2 main
+1 extended
−1 extended
+2 extended
0 extended

Data Referensi Lanjutan

Konstanta Pemerisaian (3)
nOrbitalσ
1s0,3421
2p3,5468
2s3,5084
Detail Jari-jari Kristal (5)
MuatanCNSpinrcrystal (pm)Asal
-2II121
-2III122
-2IV124
-2VI126
-2VIII128
Mode Peluruhan Isotop (22)
IsotopModeIntensitas
112p100%
122p100%
13B+100%
13B+p10,9%
14B+100%
15B+100%
19B-100%
20B-100%
21B-100%
21B-n—
Faktor Hamburan Sinar-X (502)
Energi (eV)f₁f₂
10—0,70328
10,1617—0,70723
10,3261—0,70738
10,4931—0,70753
10,6628—0,70768
10,8353—0,70783
11,0106—0,70798
11,1886—0,70813
11,3696—0,70828
11,5535—0,70843

Data Tambahan

Sources

Sources of this element.

Oxygen is the third most abundant element found in the sun, and it plays a part in the carbon-nitrogen cycle, the process once thought to give the sun and stars their energy. Oxygen under excited conditions is responsible for the bright red and yellow-green colors of the Aurora Borealis.

A gaseous element, oxygen forms 21% of the atmosphere by volume and is obtained by liquefaction and fractional distillation. The atmosphere of Mars contains about 0.15% oxygen. The element and its compounds make up 49.2%, by weight, of the earth's crust. About two thirds of the human body and nine tenths of water is oxygen.

In the laboratory it can be prepared by the electrolysis of water or by heating potassium chlorate with manganese dioxide as a catalyst.

Referensi (1)

Isotopes in Forensic Science and Anthropology

Information on the use of this element's isotopes in forensic science and anthropology.

Measurements of relative 18O abundances have been used to determine the breeding grounds of many species of migrant songbirds. These species of songbirds only grow their feathers before migration, and they grow them on or close to their breeding grounds. Therefore, the isotopic composition of a bird’s feathers correlates to the isotopic signature of the growing season’s precipitation [19] K. A. Hobson. Oecologia120, 314 (1999)., [20] K. A. Hobson, L. I. Wassenaar. Oecologia.109, 142 (1996)..

Measurements of relative 18O abundances of human hair or nail samples collected at archeological sites have been used to determine the geographic region in which a subject lived based on the oxygen isotopic composition of the water they drank (Fig. IUPAC.8.3). This is possible because hair stores a daily record of oxygen isotopic composition of intake water, which correlates to local meteoric water [92] D. M. O’Brien, M. J. Woller. Rapid Commun. Mass Spectrom.21, 2422 (2007)..

Referensi (7)
  • [14] W. Dansgaard. Tellus16, 436 (1964).
  • [15] I. D. Clark, P. Fritz. Environmental Isotopes in Hydrogeology, p. 328, Lewis Publishers, New York (1997).
  • [19] K. A. Hobson. Oecologia120, 314 (1999).
  • [20] K. A. Hobson, L. I. Wassenaar. Oecologia.109, 142 (1996).
  • [92] D. M. O’Brien, M. J. Woller. Rapid Commun. Mass Spectrom.21, 2422 (2007).
  • [93] I. Fraser, W. Meier-Augenstein, R. M. Kalin. Rapid Commun. Mass Spectrom.20, 1109 (2006).
  • [4] IUPAC Periodic Table of the Elements and Isotopes (IPTEI) https://doi.org/10.1515/pac-2015-0703

Referensi

(9)
2 Atomic Mass Data Center (AMDC), International Atomic Energy Agency (IAEA)
O

The half-life and atomic mass data was provided by the Atomic Mass Data Center at the International Atomic Energy Agency.

3 IUPAC Commission on Isotopic Abundances and Atomic Weights (CIAAW)
Oxygen

Element data are cited from the Atomic weights of the elements (an IUPAC Technical Report). The IUPAC periodic table of elements can be found at https://iupac.org/what-we-do/periodic-table-of-elements/. Additional information can be found within IUPAC publication doi:10.1515/pac-2015-0703 Copyright © 2020 International Union of Pure and Applied Chemistry.

4 IUPAC Periodic Table of the Elements and Isotopes (IPTEI)

The information are cited from Pure Appl. Chem. 2018; 90(12): 1833-2092, https://doi.org/10.1515/pac-2015-0703.

Catatan lisensi: Copyright (c) 2020 International Union of Pure and Applied Chemistry. The International Union of Pure and Applied Chemistry (IUPAC) contribution within Pubchem is provided under a CC-BY-NC-ND 4.0 license, unless otherwise stated.
5 Jefferson Lab, U.S. Department of Energy
Oxygen

Thomas Jefferson National Accelerator Facility (Jefferson Lab) is one of 17 national laboratories funded by the U.S. Department of Energy. The lab's primary mission is to conduct basic research of the atom's nucleus using the lab's unique particle accelerator, known as the Continuous Electron Beam Accelerator Facility (CEBAF). For more information visit https://www.jlab.org/

Catatan lisensi: Please see citation and linking information: https://education.jlab.org/faq/index.html
6 Los Alamos National Laboratory, U.S. Department of Energy
Oxygen

The periodic table at the LANL (Los Alamos National Laboratory) contains basic element information together with the history, source, properties, use, handling and more. The provenance data may be found from the link under the source name.

7 NIST Physical Measurement Laboratory
Oxygen

The periodic table contains NIST's critically-evaluated data on atomic properties of the elements. The provenance data that include data for atomic spectroscopy, X-ray and gamma ray, radiation dosimetry, nuclear physics, and condensed matter physics may be found from the link under the source name. Ref: https://www.nist.gov/pml/atomic-spectra-database

8 PubChem Elements
Oxygen

This section provides all form of data related to element Oxygen.

9 PubChem Elements
Oxygen

The element property data was retrieved from publications.

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