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A NUCLEOSIDE UNDER OBSERVATION

IN THE GAS PHASE: A ROTATIONAL

STUDY OF URIDINE

I. PEÑA, J.L. ALONSO

Grupo de Espectroscopia Molecular. Unidad asociada CSIC

Laboratorios de Espectroscopia y Bioespectroscopia

Edificio Quifima. Parque Científico

Universidad de Valladolid SPAIN

Introduction

 Nucleosides bound to one or more phosphate groups

(nucleotides) are considered the molecular building blocks of DNA and RNA

 A nucleoside is composed of a nitrogen base bound to either ribose or deoxyribose via a beta-glycosidic linkage.

In particular, uridine is composed of uracil and ribose

 The jet-cooled rotational spectrum of uracil has been investigated using LA-MB-FTMW spectroscopy.

1 The diketo structure of uracil has been determined

H

O

H

O

H

N

3

O

H

H

N

O

H

N

H

N

O

N

1

H

DIKETO FORM

O

H

[1]J. Phys. Chem. A, 111, 3443 (2007)

N

O

N O

H H

PLAUSIBLE TAUTOMERS OF URACIL

N

HO

H

O

N

NH

O

URACIL

H

H

OH

O

H

OH

H

GLYCOSIDIC BOND

RIBOSE

URIDINE

Introduction

 For D-ribose, eight different PYRANOSE FORMS have been recently characterized in gas phase using

CP-FTMW spectroscopy + Laser Ablation

Uridine: the simplest nucleoside

H

O

N

H

NH

O

The most stable form of URACIL

H

OH

H

H

OH

O

H

OH

H

OH +

H

H

H

H

O

H

H

OH OH

OH OH

The most stable  and

β forms of RIBOSE

Why did nature choose the furanose and not the pyranose form of ribose in RNA????

O

NH

N

H

H

OH

H

H

OH

O

H

OH

H

O

O

NH

N O

HO

H

H

OH

O

H

OH

H

URIDINE

Furanose form of ribose in RNA

Uridine: the simplest nucleoside

Some structural arguments could be based on the intramolecular interactions between the base and ribose moieties, which would stabilize the furanose form versus the pyranose form

The aim of the present work is the observation of the isolated nucleoside uridine in the gas phase, free from the bulk effects of the native envinroment, to reveal the biologically important uracil/ribose intramolecular interactions

Experimental: CP-FTMW + Laser Ablation

A commercial sample of uridine (m.p.: 163-167ºC) was vaporized using the third harmonic of a 20 ps Nd:YAG laser. Products of the laser ablation were supersonically expanded in Ne and probed by broadband CP-FTMW

6-12GHz

120000 fids

6000 7000 8000 9000 10000 11000 12000

 / MHz

CP-FTMW + LA at GEM, Valladolid

S. Mata I. Peña, et al. J. Mol. Spectr. 280(2012) 91–96

Uridine: CP-FTMW rotational spectra

PHOTOFRAGMENTATION PRODUCTS

2

Uracil

12

1

01

HC

3

N

7870 7875

 /MHz

7880 7885

Photofragmentation products such as uracil, glyceraldehyde, ethylene glycol, acetic acid, oxoacetic acid, formaldehyde, acrolein and cyanoacetylene seem to be dominant in the spectrum

6000 7000 8000 9000 10000 11000 12000

 / MHz

120000 fids

Is neutral uridine present in the supersonic expansion in an appreciable amount to be detected?

Uridine: CP-FTMW rotational spectra

6000

Resultant spectrum without photofragmentation products

7000

10

19

9

18 transition

8000 rotational

6075

 /MHz

6080

9000

 / MHz

10000 11000

Assignment of

 a and

 b

-type R-branch progressions (with the quantum number J ranging from 4 to 17), as corresponding to one rotamer

12000

4

3

12

18

3

2

11

6

4

6

13

5

10

15

17

17

10

9

12

13

16

16

5

11

12

15

16

16

10

15

15

12

11

10

9

K’

+1

10

8

5

5

3

0

5

5

4

4

5

5

3

5

0

1

5

2

4

2

6

6

4

3

0

1

0

1

2

0

0

3

3

0

4

5

5

K

-1

4

5

J’

15

16

17

17

15

15

15

15

16

16

8

14

14

15

16

16

15

14

14

14

14

13

13

13

15

8

8

15

18

7

7

15

9

16

9

9

10

J’’

14

15

16

16

14

14

14

14

15

15

7

13

13

14

15

15

14

13

13

13

13

12

12

12

14

7

7

14

17

6

6

14

8

8

9

15

8

 obs

7973.81400

7977.91480

8265.73370

8302.35480

8305.31120

8454.27510

8587.26500

8591.03200

8612.29900

8694.26730

8302.35480

8843.46960

8844.42330

8845.13850

8846.09220

8886.52800

8913.66000

9188.03220

9190.89320

9196.13840

9233.66550

9254.50330

9295.98810

9384.15530

9385.63350

9438.03790

9440.89890

9491.01450

9491.63440

9544.75400

9924.60250

10095.35790

10097.55130

10156.34540

10696.12500

10702.75310

11290.59790

4

4

3

1

4

4

4

3

4

4

3

4

1

0

5

1

4

2

6

6

3

3

0

0

1

1

2

1

0

3

3

1

4

5

5

K

-1

’’ K

+1

’’

4

5

9

7

3

4

11

17

2

3

10

5

5

5

12

4

9

14

16

16

9

8

11

12

15

15

4

10

11

14

15

15

9

14

14

11

10

9

8

Results

Parameter

A /MHz

B /MHz

C /MHz

 μ

 μ

 μ c a b

/D

/D

/D

14 N(1)

/MHz

 aa bb cc

/MHz

/MHz

14 N(3)

 aa

/MHz

 bb

 cc

/MHz

/MHz

N c

ΔE /cm -1

EXPERIMENT

Rotamer

886.0063 (24) d

335.59351 (71)

270.10754 (36)

THEORY

NOT CONCLUSIVE IDENTIFICATION Anti/C2’endo t

Syn/C3’endo g+

901.2

935.8

790.0

799.7

925.5

340.6

276.6

308.4

266.6

352.6

261.4

330.6

262.9

300.4

264.0

Observed

Observed

Observed

2.1

3.7

1.6

2.8

3.1

1.5

0.9

0.7

0.8

4.5

0.9

1.3

2.3

2.3

0.2

-

-

-

66

-

-

-

-

1.50

1.43

-2.93

1.74

1.11

-2.85

-

0

1.82

0.73

-2.56

2.03

0.47

-2.50

-

383

1.48

1.71

-3.19

1.78

1.34

-3.12

-

664

1.46

1.81

-3.27

1.62

1.51

-3.13

-

701

1.82

-0.72

-1.11

1.98

-0.75

-1.23

-

751

1 Ab initio calculations MP2-6-311++G(d,p) below 1000 cm -1

Experimental: narrowband LA-MB-FTMW

• 3-10GHz

• Third harmonic of a 20 picosecond laser

• Microwave radiation pulse of 0.3

 s duration

• Frequency accuracy better than 5 kHz and an estimated resolution of 7 kHz

FT-MW

10

19

6075

 /MHz

6080

9

18

Broadband CP-FTMW rotational transition

Fabry-Pérot Resonator

Picosecond Laser

LA-MB-FTMW at GEM, Valladolid

I.

Peña et al. JACS 134 (2012) 2305 – 2312

6079.5

2,9 2,8

2,8 2,7

1,10 1,9

0,10 0,9

6080.0

 / MHz

1,11 1,10

O

NH

14 N

2,10 2,9

6080.5

HO

H

H

OH

O

H

OH

H

N

14 N

O

Narrowband LA-MB-FTMW

Sub-Doppler resolution

Results

Parameter

A /MHz

B /MHz

C /MHz

D

 μ

J

/kHz

 μ b a

/D

 μ c

/D

/D

14 N(1)

/MHz

 aa bb cc

/MHz

/MHz

14 N(3)

 aa

/MHz

 bb

 cc

/MHz

/MHz

N c

ΔE /cm -1

EXPERIMENT

Rotamer

885.98961 (14) d

335.59720 (35)

270.11270 (20)

0.0115 (10)

Observed

Observed

Observed

THEORY

Anti/C2’endo g+ 1 Syn/C2’endo g+

Anti/C3’endo g+ Anti/C2’endo t

Syn/C3’endo g+

901.2

340.6

276.6

-

2.1

3.7

0.9

935.8

308.4

266.6

-

1.6

2.8

0.7

790.0

352.6

261.4

-

3.1

1.5

799.7

330.6

262.9

-

4.5

0.9

1.3

925.5

300.4

264.0

-

2.3

2.3

0.2

1.540 (42)

1.456 (72)

-2.996 (72)

1.719 (40)

1.261 (70)

-2.979 (70)

47

1.50

1.43

-2.93

1.74

1.11

-2.85

0

1.82

0.73

-2.56

2.03

0.47

-2.50

383

1.48

1.71

-3.19

1.78

1.34

-3.12

664

1.46

1.81

-3.27

1.62

1.51

-3.13

701

1.82

-0.72

-1.11

1.98

-0.75

-1.23

751

1 Ab initio calculations MP2-6-311++G(d,p) below 1000 cm -1

1. Distances in Å

Intramolecular hydrogen bonding

2.97

Intramolecular hydrogen bonding network: 1

O3  H  O2  H  O2

Weak interactions:

C2  H  O5 

C6  H  O5 

Anti/C2’ -endo g+

Conclusions

 Uridine has been placed in the gas phase by laser ablation and the most stable Anti/C2-endo g+ has been characterized by broadband CP-FTMW and narrowband LA-MB-FTMW

 The observation of this conformer is in accordance with ab initio results, but in relative contrast with those obtained by X-ray 1 where C3 ’endo/anti conformation has been observed. It has been shown that the C3 ’ -endo configuration, which is in RNA, is favored when an explicit water molecule is introduced into the calculation. Nevertheless, previous calculations indicate that the change of the sugar pucker from

C3 ’ -endo to C2 ’ -endo in single-stranded RNA is energetically possible

 The preference for furanoses in RNA might be due to the observed intramolecular hydrogen bond network and the weak interactions between uracil and ribose, which over stabilizes this species and prevents the generation of pyranoses.

1. E. A. Green et al., Acta Cryst. (1975), B31, 102

ACKNOWLEDGMENTS

Grupo de Espectroscopia Molecular (GEM)

Laboratorios de Espectroscopia y

Bioespectroscopia, Unidad Asociada CSIC,

UVa,Valladolid, Spain

Grants CTQ 2010- 19008,

AYA 2009-07304 and AYA 2012-32032

CSD 2009-00038 Molecular Astrophysics

Grants VA070A08 and CIP13/01

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